Dust Grain Size Distributions and Extinction in the Milky Way, LMC, and SMC

Abstract

We construct size distributions for carbonaceous and silicate grain populations in different regions of the Milky Way, LMC, and SMC. The size distributions include sufficient very small carbonaceous grains (including polycyclic aromatic hydrocarbon molecules) to account for the observed infrared and microwave emission from the diffuse interstellar medium. Our distributions reproduce the observed extinction of starlight, which varies depending upon the interstellar environment through which the light travels. As shown by Cardelli, Clayton & Mathis in 1989, these variations can be roughly parameterized by the ratio of visual extinction to reddening, R_V. We adopt a fairly simple functional form for the size distribution, characterized by several parameters. We tabulate these parameters for various combinations of values for R_V and b_C, the C abundance in very small grains. We also find size distributions for the line of sight to HD 210121, and for sightlines in the LMC and SMC. For several size distributions, we evaluate the albedo and scattering asymmetry parameter, and present model extinction curves extending beyond the Lyman limit.

Latex (44 pages, 24 figures), replaced with final journal version

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• Feedback-Free Starbursts at Cosmic Dawn: Observable Predictions for JWST
• Observational Constraints on Submillimeter Dust Opacity
• The Dielectric Function of "Astrodust" and Predictions for Polarization in the 3.4$\mu$m and 10$\mu$m Features
• Predictions for the spatial distribution of the dust continuum emission in 1<z<5 star-forming galaxies
• Non-equilibrium chemistry and cooling in the diffuse interstellar medium - I. Optically thin regime
• Non-equilibrium chemistry and cooling in the diffuse interstellar medium - II. Shielded gas
• Optical Characterization of a New Young Stellar Population in the Serpens Molecular Cloud
• Water in star-forming regions with Herschel: highly excited molecular emission from the NGC 1333 IRAS 4B outflow
• The Case of AB Aurigae's Disk in Polarized Light: Is There Truly a Gap?
• On the origin of the spiral morphology in the Elias 2-27 circumstellar disc
• Reflections on Reflexions: I. Light Echoes in Type Ia Supernovae
• The Inner Rim of YSO Disks: Effects of dust grain evolution
• Spiral arms in the proto-planetary disc HD100453 detected with ALMA: evidence for binary-disc interaction and a vertical temperature gradient
• Gaps, rings, and non-axisymmetric structures in protoplanetary disks - Emission from large grains
• Dust in the Circumgalactic Medium of Low-Redshift Galaxies
• Molecular Line Emission from Massive Protostellar Disks: Predictions for ALMA and the EVLA
• Decomposing Dusty Galaxies. I. Multi-Component Spectral Energy Distribution Fitting
• Photoelectric Emission from Dust Grains Exposed to Extreme Ultraviolet and X-ray Radiation
• Cloudshine: New Light on Dark Clouds
• Polarization of Dust Emission in Clumpy Molecular Clouds and Cores
• XMM-Newton observation of 4U 1820-30: Broad band spectrum and the contribution of the cold interstellar medium
• A Resolved Debris Disk around the G2V star HD 107146
• UV dust attenuation in spiral galaxies: the role of age-dependent extinction and of the IMF
• On the Origin of Stellar Masses
• The Embedded Super Star Cluster of SBS0335-052
• The effect of stellar feedback on the formation and evolution of gas and dust tori in AGN
• Dust input from AGB stars in the Large Magellanic Cloud
• Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments
• Mid-Infrared Extinction and its Variation with Galactic Longitude
• Observed sizes of planet-forming disks trace viscous evolution
• HD and H2 formation in low-metallicity dusty gas clouds at high redshift
• Spitzer spectral line mapping of supernova remnants: I. Basic data and principal component analysis
• H-alpha emission in local galaxies: star formation, time variability and the diffuse ionized gas
• The Thermal Structure of Gas in Pre-Stellar Cores: A Case Study of Barnard 68
• Tree-based solvers for adaptive mesh refinement code FLASH - I: gravity and optical depths
• SCUBA and Spitzer observations of the Taurus molecular cloud - pulling the bull's tail
• HD far infrared emission as a measure of protoplanetary disk mass
• Radiation Feedback in ULIRGS: Are Photons Movers and Shakers?
• Observability of Scattered-Light Echoes Around Variable Stars and Cataclysmic Events
• Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at $z=5.85$
• The Three-Dimensional Circumstellar Environment of SN 1987A
• Phosphorus in the Young Supernova Remnant Cassiopeia A
• IRS Spectra of Solar-Type Stars: \break A Search for Asteroid Belt Analogs
• The properties of the 2175AA extinction feature discovered in GRB afterglows
• Outflow-Confined H II Regions. I. First Signposts of Massive Star Formation
• SpeX near-infrared spectroscopic extinction curves in the Milky Way
• Mixed aliphatic and aromatic composition of evaporating very small grains in NGC 7023 revealed by the 3.4/3.3 $\mu$m ratio
• Physical Processes in Star Formation
• Very Large Interstellar Grains as Evidenced by the Mid-Infrared Extinction
• Spitzer mapping of molecular hydrogen pure rotational lines in NGC 1333: A detailed study of feedback in star formation
• Extended silicate dust emission in PG QSOs
• Azimuthal Density Variations Around the Rim of Tycho's Supernova Remnant
• Coagulation and Fragmentation in molecular clouds. II. The opacity of the dust aggregate size distribution
• Expanding bubbles in Orion A: [CII] observations of M42, M43, and NGC 1977
• Hubble and Spitzer Observations of an Edge-on Circumstellar Disk around a Brown Dwarf
• The Role of Polycyclic Aromatic Hydrocarbons in Ultraviolet Extinction. I. Probing small molecular PAHs
• Photometry of the Type Ia Supernovae 1999cc, 1999cl, and 2000cf
• Carbon Fractionation in PDRs
• An evolving compact jet in the black hole X-ray binary MAXI J1836-194
• CO line emission from galaxies in the Epoch of Reionization
• Evolution of dust and ice features around FU Orionis objects
• Attenuation caused by a distant Isothermal Turbulent Screen
• The effect of local optically thick regions in the long-wave emission of young circumstellar disks
• The Infrared Extinction Law at Extreme Depth in a Dark Cloud Core
• Warm dust in high-z galaxies: origin and implications
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• The Submm and mm Excess of the SMC: Magnetic Dipole Emission from Magnetic Nanoparticles?
• Diverse Structural Evolution at z > 1 in Cosmologically Simulated Galaxies
• IGM metal enrichment through dust sputtering
• The THESAN project: ionizing escape fractions of reionization-era galaxies
• Dust scaling relations in a cosmological simulation
• Detection of Structure in Infrared-Dark Clouds with Spitzer: Characterizing Star Formation in the Molecular Ring
• Mid-Infrared Properties of the Swift Burst Alert Telescope Active Galactic Nuclei Sample of the Local Universe. I. Emission-Line Diagnostics
• The ALMA view of GMCs in NGC 300: Physical Properties and Scaling Relations at 10 pc Resolution
• The opaque nascent starburst in NGC 1377: Spitzer SINGS observations
• Measurements of the Intensity and Polarization of the Anomalous Microwave Emission in the Perseus molecular complex with QUIJOTE
• Modeling the Anomalous Microwave Emission with Spinning Nanoparticles: No PAHs Required
• Infrared emission from tidal disruption events --- probing the pc-scale dust content around galactic nuclei
• A self-consistent model of Galactic stellar and dust infrared emission and the abundance of polycyclic aromatic hydrocarbons
• The Polycyclic Aromatic Hydrocarbon Mass Fraction on a 10 pc scale in the Magellanic Clouds
• Detections of the 2175 ÅDust Feature at 1.4z 1.5 from the Sloan Digital Sky Survey
• Preparing for low surface brightness science with the Vera C. Rubin Observatory: characterisation of tidal features from mock images
• Inferring giant planets from ALMA millimeter continuum and line observations in (transition) disks
• The dust-continuum size of TNG50 galaxies at $z=1-5$: a comparison with the distribution of stellar light, stars, dust and H${}_2$
• Large dust grains in the inner region of circumstellar disks
• The Impact of Feedback During Massive Star Formation by Core Accretion
• Chemical evolution of protoplanetary disks - the effects of viscous accretion, turbulent mixing and disk winds
• Interstellar ices as witnesses of star formation: selective deuteration of water and organic molecules unveiled
• High resolution spectroscopy of Ne II emission from young stellar objects
• CARMA interferometric observations of 2MASS J044427+2512: the first spatially resolved observations of thermal emission of a brown dwarf disk
• Estimating gas masses and dust-to-gas ratios from optical spectroscopy
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• Forces on Dust Grains Exposed to Anisotropic Interstellar Radiation Fields
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• The Spitzer survey of interstellar clouds in the Gould Belt. II. The Cepheus Flare observed with IRAC and MIPS
• The SDSS-2MASS-WISE Ten Dimensional Stellar Color Locus
• Absorption and scattering by interstellar dust: XMM-Newton observation of Cyg X-2
• Escape of Lyman-alpha and continuum photons from star-forming galaxies
• A Shock Flash Breaking Out of a Dusty Red Supergiant
• Gas-phase recombination, grain neutralization and cosmic-ray ionization in diffuse gas
• Cool dust heating and temperature mixing in nearby star-forming galaxies
• Mid-infrared spectral evidence for a luminous dust enshrouded source in Arp220
• Distinguishing Mergers and Disks in High Redshift Observations of Galaxy Kinematics
• Simulations of Dust in Interacting Galaxies I: Dust Attenuation
• CO2 infrared emission as a diagnostic of planet-forming regions of disks
• Dynamical Expansion of Ionization and Dissociation Front around a Massive Star. I. A Mode of Triggered Star Formation
• Horizon-AGN virtual observatory - 1. SED-fitting performance and forecasts for future imaging surveys
• A dynamical constraint on interstellar dust models from radiative torque disruption
• Structuring the HD 141569 A circumstellar dust disk. Impact of eccentric bound stellar companions
• The Spitzer c2d Survey of Nearby Dense Cores: IV. Revealing the Embedded Cluster in B59
• A New Spin on Galactic Dust
• Spatially resolved mid-infrared observations of the triple system T Tauri
• Spitzer IRAC Images and Sample Spectra of Cassiopeia A's Explosion
• Evidence for dust evolution within the Taurus Complex from Spitzer images
• Modeling the Dust Properties of z ~ 6 Quasars with ART^2 -- All-wavelength Radiative Transfer with Adaptive Refinement Tree
• PACS and SPIRE photometer maps of M33: First results of the Herschel M33 extended survey (HERM33ES)
• Dust temperature in ALMA $\hbox{[C $\scriptstyle\rm II $]}$-detected high-$z$ galaxies
• A Spitzer Survey of Protoplanetary Disk Dust in the Young Serpens Cloud: How do Dust Characteristics Evolve with Time?
• Locating the planetesimals belts in the multiple-planet systems HD 128311, HD 202206, HD 82943 and HR 8799
• The most distant, luminous, dusty star-forming galaxies: redshifts from NOEMA and ALMA spectral scans
• Molecular hydrogen formation on dust grains in the high redshift universe
• ALMA observations of fragmentation, sub-structure, and protostars in high-mass starless clump candidates
• The Enigmatic Young Low-Mass Variable TWA 30
• Panchromatic observations and modeling of the HV Tau C edge-on disk
• Shells of dust around AGB stars: effects on the integrated spectrum of Single Stellar Populations
• Discovery of superthermal hydroxyl (OH) in the HH211 outflow
• Using the X-ray Dust Scattering Halo of Cygnus X-1 to determine distance and dust distributions
• Parameterizing the interstellar dust temperature
• Is the dust-to-gas ratio constant in molecular clouds?
• A multi-wavelength scattered light analysis of the dust grain population in the GG Tau circumbinary ring
• The Disc Miner I: A statistical framework to detect and quantify kinematical perturbations driven by young planets in discs
• Inclination-Dependent Extinction Effects in Disk Galaxies in the Sloan Digital Sky Survey
• FUSE Measurements of Far Ultraviolet Extinction. II. Magellanic Cloud Sight Lines
• 'Super-Chandrasekhar' Type Ia Supernovae at nebular epochs
• ART^2 : Coupling Lyman-alpha Line and Multi-wavelength Continuum Radiative Transfer
• The X-ray Halo of GX 13+1
• The role of the charge state of PAHs in ultraviolet extinction
• Gas and multi-species dust dynamics in viscous protoplanetary discs: the importance of the dust back-reaction
• Benchmarking the Calculation of Stochastic Heating and Emissivity of Dust Grains in the Context of Radiative Transfer Simulations
• Mid-infrared spectra of optically selected type 2 quasars
• The T Tauri star RY Tau as a case study of the inner regions of circumstellar dust disks
• A Massive Shell of Supernova-formed Dust in SNR G54.1+0.3
• ALMA observations of the debris disk around the young Solar Analog HD 107146
• Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties
• Time-resolved infrared emission from radiation-driven central obscuring structures in Active Galactic Nuclei
• ALMA observations of rho-Oph 102: grain growth and molecular gas in the disk around a young Brown Dwarf
• Photoprocessing of H2S on dust grains: building S chains in translucent clouds and comets
• Waves on the surface of the Orion molecular cloud
• The Dynamics, Destruction, and Survival of Supernova-Formed Dust Grains
• Gamma-ray burst optical light-curve zoo: comparison with X-ray observations
• A 30 AU radius CO gas hole in the disk around the Herbig Ae star Oph IRS 48
• Astrophysical Shrapnel: Discriminating Among Near-Earth Stellar Explosion Sources of Live Radioactive Isotopes
• Shock processing of interstellar dust and polycyclic aromatic hydrocarbons in the supernova remnant N132D
• Determining the Distance of Cyg X-3 with its X-ray Dust Scattering Halo
• The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from the TNG50 simulation in comparison to MUSE observations
• The dust, planetesimals and planets of HD 38529
• The Bolocam Galactic Plane Survey -- III. Characterizing Physical Properties of Massive Star-Forming Regions in the Gemini OB1 Molecular Cloud
• A Multiwavelength Look at Galactic Massive Star Forming Regions
• Dust formation in the ejecta of the Type II-P supernova 2004dj
• Impact of grain evolution on the chemical structure of protoplanetary disks
• Infrared and X-Ray Evidence for Circumstellar Grain Destruction by the Blast Wave of Supernova 1987A
• Powderday: Dust Radiative Transfer for Galaxy Simulations
• Molecular Gas and the Young Starburst in NGC 5253, Revisited
• Mapping the Dynamics of a Giant Ly-alpha Halo at z=4.1 with MUSE: The Energetics of a Large Scale AGN-Driven Outflow around a Massive, High-Redshift Galaxy
• Mapping warm molecular hydrogen with Spitzer's Infrared Array Camera (IRAC)
• Remodeling the evolution of grain size distribution in galaxies
• Adaptive Optics Imaging of the AU Microscopii Circumstellar Disk: Evidence for Dynamical Evolution
• Long-wavelength observations of debris discs around sun-like stars
• FitSKIRT: genetic algorithms to automatically fit dusty galaxies with a Monte Carlo radiative transfer code
• Interstellar Dust in the Solar System
• The circumstellar disc in the Bok globule CB 26: Multi-wavelength observations and modelling of the dust disc and envelope
• Measurements of water surface snow lines in classical protoplanetary disks
• JCMT BISTRO survey: Magnetic Fields within the Hub-Filament Structure in IC 5146
• Ro-vibrational excitation of an organic molecule (HCN) in protoplanetary disks
• The Dark Energy Camera Plane Survey 2 (DECaPS2): More Sky, Less Bias, and Better Uncertainties
• Constraints on the radial distribution of the dust properties in the CQ Tau protoplanetary disk
• Mineral Processing by Short Circuits in Protoplanetary Disks
• Formation and Evolution of Planetary Systems: Cold Outer Disks Associated with Sun-like stars
• SEEDS Adaptive Optics Imaging of the Asymmetric Transition Disk Oph IRS 48 in Scattered Light
• The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. I. Chamaeleon II Observed with MIPS
• Star Formation and Clumps in Cosmological Galaxy Simulations with Radiation Pressure Feedback
• The Bolocam Galactic Plane Survey. VIII. A Mid-Infrared Kinematic Distance Discrimination Method
• Grain alignment and disruption by radiative torques in dense molecular clouds and implication for polarization holes
• The accumulation and trapping of grains at planet gaps: effects of grain growth and fragmentation
• The effects of dust on the derived photometric parameters of disks and bulges in spiral galaxies
• The missing gas problem in GRB host galaxies: evidence for a highly ionised component
• Interstellar Gas-phase Element Depletions in the Small Magellanic Cloud: A Guide to Correcting for Dust in QSO Absorption Line Systems
• A dust and gas cavity in the disc around CQ Tau revealed by ALMA
• Physical properties of Southern infrared dark clouds
• Two-size approximation: a simple way of treating the evolution of grain size distribution in galaxies
• Infrared Spectroscopic Survey of the Quiescent Medium of Nearby Clouds: I. Ice Formation and Grain Growth in Lupus
• Establishing binarity amongst Galactic RV Tauri stars with a disc
• Three dimensional interstellar extinction map towards the Galactic Bulge
• The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-Forming Region
• Gemini Imaging of Mid-IR Emission from the Nuclear Region of Centaurus A
• Interrogating Seyferts with NebulaBayes: Spatially probing the narrow-line region radiation fields and chemical abundances
• Impact of Lyman alpha pressure on metal-poor dwarf galaxies
• On the AU Mic debris disk: density profiles, grain properties and dust dynamics
• The Formation and Evolution of Planetary Systems (FEPS): Discovery of an Unusual Debris System Associated with HD 12039
• Dust processing in photodissociation regions - Mid-IR emission modelling
• Formation History of Polycyclic Aromatic Hydrocarbons in Galaxies
• The Magellanic Quasars Survey. III. Spectroscopic Confirmation of 758 AGNs Behind the Magellanic Clouds
• The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation
• Spitzer observations of the Hyades: Circumstellar debris disks at 625 Myr of age
• Pégase.3: A code for modeling the UV-to-IR/submm spectral and chemical evolution of galaxies with dust
• The Infrared Emission from the Narrow Line Region
• DIGIT survey of far-infrared lines from protoplanetary discs: II. CO
• Starburst Galaxies: Why the Calzetti Dust Extinction Law?
• Ultraviolet Extinction at High Galactic Latitudes
• Molecular Line Observations of Infrared Dark Clouds: Seeking the Precursors to Intermediate and Massive Star Formation
• Interpreting the evolution of galaxy colours from $z=8$ to $z=5$
• Dust properties in M31.I.Basic properties and a discussion on age-dependent dust heating
• LIDA - The Leiden Ice Database for Astrochemistry
• Dust properties inside molecular clouds from coreshine modeling and observations
• The physics of Lyman-alpha escape from disc-like galaxies
• Empirical calibration of the reddening maps in the Magellanic Clouds
• Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
• Using M Dwarf Spectra to Map Extinction in the Local Galaxy
• Observation of the Far-ultraviolet Continuum Background with SPEAR/FIMS
• Fervent: Chemistry-coupled, ionising and non-ionising radiative feedback in magnetohydrodynamical simulations
• Redshift and luminosity evolution of the intrinsic alignments of galaxies in Horizon-AGN
• Multi-epoch Ultraviolet HST Observations of Accreting Low-mass Stars
• The chemistry of disks around T Tauri and Herbig Ae/Be stars
• UV-driven chemistry in simulations of the interstellar medium. I. Post-processed chemistry with the Meudon PDR code
• Extragalactic Imprints in Galactic Dust Maps
• Analytical Formulas of Molecular Ion Abundances and N2H+ Ring in Protoplanetary Disks
• The infrared-dark dust content of high redshift galaxies
• Dust Evolution in Galaxy Cluster Simulations
• Spectral Energy Distributions of Circumstellar Debris Disks I. Analytic Disk Density Distributions
• GIARPS High-resolution Observations of T Tauri stars (GHOsT). IV. Accretion properties of the Taurus-Auriga young association
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• The Orion HII Region and the Orion Bar in the Mid-Infrared
• The merger-driven evolution of warm infrared luminous galaxies
• Spectacular Spitzer images of the Trifid Nebula: Protostars in a young, massive-star-forming region
• Galaxy simulation with the evolution of grain size distribution
• Multi-wavelength modeling of the spatially resolved debris disk of HD 107146
• The Spitzer c2d Survey of Nearby Dense Cores. IX. Discovery of a Very Low Luminosity Object Driving a Molecular Outflow in the Dense Core L673-7
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Photoelectric cross-sections of gas and dust in protoplanetary disks
• Chemical complexity in high-mass star formation: An observational and modeling case study of the AFGL 2591 VLA 3 hot core
• An Empirical Determination of the Dust Mass Absorption Coefficient, ${\kappa }_d$, Using the Herschel Reference Survey
• The First Maps of ${\kappa }_d$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
• Reverberation in tidal disruption events: dust echoes, coronal emission lines, multi-wavelength cross-correlations, and QPOs
• Molecular line emission from a protoplanetary disk irradiated externally by a nearby massive star
• The effect of temperature mixing on the observable (T,beta)-relation of interstellar dust clouds
• Blowing in the wind: The dust wave surrounding $\sigma$ Ori AB
• Perspectives on Interstellar Dust Inside and Outside of the Heliosphere
• Analysis of the dust evolution in the circumstellar disks of TTauri stars
• Hertzsprung-Russell diagram and mass distribution of barium stars
• The interaction of relativistic spacecrafts with the interstellar medium
• Star Forming Galaxies as AGN Imposters? A Theoretical Investigation of the Mid-infrared Colors of AGNs and Extreme Starbursts
• Evolution of dust extinction curves in galaxy simulation
• Lack of PAH emission toward low-mass embedded young stellar objects
• Apparent disk-mass reduction and planetesimal formation in gravitationally unstable disks in Class 0/I YSOs
• SOFIA mid-infrared observations of Supernova 1987A in 2016 --- forward shocks and possible dust re-formation in the post-shocked region?
• Spectroscopic properties of Young Stellar Objects in the Lupus Molecular Clouds
• Photodissociation Region Diagnostics Across Galactic Environments
• The molecular complex associated with the Galactic HII region Sh2-90: a possible site of triggered star formation
• Modeling UV Radiation Feedback from Massive Stars: III. Escape of Radiation from Star-forming Giant Molecular Clouds
• The Mid-Infrared Extinction Law and its Variation in the Coalsack Nebula
• Mass constraints for 15 protoplanetary disks from HD 1-0
• Radiation pressure confinement - IV. Application to broad absorption line outflows
• H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen
• The First Detection of Spatially Resolved Mid-Infrared Scattered Light from a Protoplanetary Disk
• The effects of dust on the photometric parameters of decomposed disks and bulges
• Modelling galaxy spectra in presence of interstellar dust. I. The model of ISM and the library of dusty SSPs
• The Circumstellar Environment of R Coronae Borealis: White Dwarf Merger or Final Helium Shell Flash?
• Vertical settling and radial segregation of large dust grains in the circumstellar disk of the Butterfly Star
• On the Origins of the High-Latitude H-alpha Background
• It's Alive! The Supernova Impostor 1961V
• Constraint on the Polarization of Electric Dipole Emission from Spinning Dust
• Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
• ALMA observations of cool dust in a low-metallicity starburst, SBS0335-052
• Is the Galactic submillimeter dust emissivity underestimated?
• An empirical study of dust properties at the earliest epochs
• Probing the dusty environment of the Seyfert 1 nucleus in NGC 3783 with MIDI/VLTI interferometry
• Carriers of the mid-IR emission bands in PNe reanalysed. Evidence of a link between circumstellar and interstellar aromatic dust
• Physical Model of Dust Polarization by Radiative Torque Alignment and Disruption and Implications for Grain Internal Structures
• A Systematic Study of the dust of Galactic Supernova Remnants I. The Distance and the Extinction
• A survey of H${}_2$O, CO${}_2$ and CO ice features towards background stars and low mass YSOs using AKARI
• The Broadband Afterglow of GRB980329
• Detection of Ultraviolet Halos around Highly Inclined Galaxies
• SPHERE dynamical and spectroscopic characterization of HD142527B
• Main-sequence stars masquerading as Young Stellar Objects in the central molecular zone
• New HST data and modeling reveal a massive planetesimal collision around Fomalhaut
• Radial variations in grain sizes and dust scale heights in the protoplanetary disk around HD 163296 revealed by ALMA polarization observation
• Mid-infrared PAH and H2 emission as a probe of physical conditions in extreme PDRs
• The Spectrum of Integrated Millimeter Flux of the Magellanic Clouds and 30-Doradus from TopHat and DIRBE Data
• Physical Conditions in the Ionized Gas of 30 Doradus
• On the Ca-strong 1991bg-like type Ia supernova 2016hnk: evidence for a Chandrasekhar-mass explosion
• Molecular Gas in Submillimetre-Faint, Star-Forming Ultraluminous Galaxies at z>1
• GAMA/H-ATLAS: The Dust Opacity - Stellar Mass Surface Density Relation for Spiral Galaxies
• The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XII. The Perseus YSO Population as Observed with IRAC and MIPS
• Interstellar extinction and interstellar polarization: old and new models
• CO Emission in Infrared-Selected Active Galactic Nuclei
• Metallicity and the Universality of the IMF
• Dust evolution in zoom-in cosmological simulations of galaxy formation
• Evolution of the extinction curves in galaxies
• Full SED fitting with the KOSMA-τ PDR code - I. Dust modelling
• A Millimetre Survey of Starburst Dominated Ultraluminous Infrared Galaxies at z~2
• Modelling clumpy PDRs in 3D - Understanding the Orion Bar stratification
• Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
• Submillimeter Structure of the Disk of the Butterfly Star
• Variation of the extinction law in the Trifid nebula
• The Number and Observability of Population III Supernovae at High Redshifts
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Twelve type II-P supernovae seen with the eyes of Spitzer
• The Spatial Distribution of Dust and Stellar Emission of the Magellanic Clouds
• Neutral gas heating by X-rays in primitive galaxies: Infrared observations of IZw18 with Herschel
• Effects of grain growth mechanisms on the extinction curve and the metal depletion in the interstellar medium
• Trajectories and Distribution of Interstellar Dust Grains in the Heliosphere
• Sensitivity of PDR Calculations to Microphysical Details
• Probing the Role of Carbon in the Interstellar Ultraviolet Extinction
• The Interstellar Oxygen Crisis, or Where Have All the Oxygen Atoms Gone?
• On Dust Extinction of Gamma-ray Burst Host Galaxies
• Optical constants of silicon carbide for astrophysical applications. II. Extending optical functions from IR to UV using single-crystal absorption spectra
• Exact results for hydrogen recombination on dust grain surfaces
• Interstellar Medium and Star Formation of Starburst Galaxies on the Merger Sequence
• Far-Infrared Spectral Energy Distributions of Embedded Protostars and Dusty Galaxies: I. Theory for Spherical Sources
• Ultraviolet to optical diffuse sky emission as seen by the Hubble Space Telescope Faint Object Spectrograph
• Moment equations for chemical reactions on interstellar dust grains
• Submillimeter flux as a probe of molecular ISM mass in high-$z$ galaxies
• The deeply embedded starburst in SBS 0335-052
• Mapping the Extinction Curve in 3D: Structure on Kiloparsec Scales
• The Dust-to-Gas Ratio in the Small Magellanic Cloud Tail
• JWST: Deuterated PAHs, PAH-nitriles, and PAH Overtone and Combination Bands I: Program Description and First Look
• An ALMA and MagAO Study of the Substellar Companion GQ Lup B
• Herschel/PACS Imaging of Protostars in the HH 1-2 Outflow Complex
• Extinction curve template for intrinsically reddened quasars
• Detection of steam in the circumstellar disk around a massive Young Stellar Object
• The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period--Luminosity Relations
• Grain size limits derived from 3.6 μm and 4.5 μm coreshine
• Properties of Dust Grains Probed with Extinction Curves
• A giant X-ray dust scattering ring around the black hole transient MAXI J1348-630 discovered with SRG/eROSITA
• Radiative equilibrium estimates of dust temperature and mass in high-redshift galaxies
• Massive Star Formation via the Collapse of Subvirial and Virialized Turbulent Massive Cores
• Extinction Correction for Type Ia Supernova Rates. I. The Model
• An Evolutionary Model For Submillimeter Galaxies
• Candidate Water Vapor Lines to Locate the H${}_2$O Snowline through High-Dispersion Spectroscopic Observations II. The Case of a Herbig Ae Star
• Cosmological Implications of a Stellar Initial Mass Function that Varies with the Jeans Mass in Galaxies
• Swift Ultraviolet Observations of Supernova 2014J in M82: Large Extinction from Interstellar Dust
• Far-infrared Observations of the Very Low-Luminosity Embedded Source L1521F-IRS in the Taurus Star-Forming Region
• Realistic mock observations of the sizes and stellar mass surface densities of massive galaxies in FIRE-2 zoom-in simulations
• Gas and dust temperature in pre-stellar cores revisited: New limits on cosmic-ray ionization rate
• Spiral arms in thermally stratified protoplanetary discs
• Photodissociation of interstellar ArH+
• Probing the role of polycyclic aromatic hydrocarbons in the photoelectric heating within photodissociation regions
• Diffuse Galactic Light in the Field of the Translucent High Galactic Latitude Cloud MBM32
• Multiple Light Echoes from Supernova 1993J
• On the Flux of Extra-Solar Dust in Earth's Atmosphere
• A new look at the infrared properties of z $\sim$ 5 galaxies
• Photoevaporation of Jeans-unstable molecular clumps
• Hydrogenation of PAH cations: a first step towards H2 formation
• Modeling dust emission in the Magellanic Clouds with Spitzer and Herschel
• A systematic study of the escape of LyC and Ly$\alpha$ photons from star-forming, magnetized turbulent clouds
• Dust dynamics and evolution in HII regions - II. Effects of dynamical coupling between dust and gas
• Small dust grain dynamics on adaptive mesh-refinement grids. I. Methods
• THEMIS 2.0: A self-consistent model for dust extinction, emission, and polarisation
• Dust attenuation evolution in $z\sim 2$-$12$ JWST galaxies
• Candidate Water Vapor Lines to Locate the H${}_2$O Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star
• Dust absorption and scattering in the silicon K-edge
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• V1647 Orionis: One Year into Quiescence
• 3D chemical structure of diffuse turbulent ISM. I. Statistics of the HI-to-H${}_2$ transition
• Warm Dust and Spatially Variable PAH Emission in the Dwarf Starburst Galaxy NGC 1705
• Hybrid Adaptive Ray-Moment Method (HARM${}^2$): A Highly Parallel Method for Radiation Hydrodynamics on Adaptive Grids
• The Impact of Accurate Extinction Measurements for X-ray Spectral Models
• The circumstellar disk of HH 30. Searching for signs of disk evolution with multi-wavelength modeling
• The X-Ray Scattering Halo Around Nova Cygni 1992: Testing a Model for Interstellar Dust
• The picture of BLR in 2.5-D FRADO: Dynamics & Geometry
• Dust processing in elliptical galaxies
• Astrochemical relevance of VUV ionization of large PAH cations
• Self-consistent modelling of aromatic dust species and extinction curves in galaxy evolution
• Evidence for Grain Growth in Molecular Clouds: A Bayesian Examination of the Extinction Law in Perseus
• The Size-Luminosity Relationship of Quasar Narrow-Line Regions
• Observations of the Near- to Mid-Infrared Unidentified Emission Bands in the Interstellar Medium of the Large Magellanic Cloud
• Tracing large-scale structures in circumstellar disks with ALMA
• The Mid-Infrared Extinction Law in the Large Magellanic Cloud
• A chemical model for the interstellar medium in galaxies
• Enhanced production of HD and D_2 molecules on small dust grains in diffuse clouds
• Absorption and scattering by interstellar dust in the silicon K-edge of GX 5-1
• Characterizing the transition from diffuse atomic to dense molecular clouds in the Magellanic clouds with [CII], [CI], and CO
• Characterizing Dust Attenuation in Local Star-Forming Galaxies: Near-Infrared Reddening and Normalization
• Efficiency of radial transport of ices in protoplanetary disks probed with infrared observations: the case of CO${}_2$
• METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. I. Overview and Initial Results
• Herschel images of NGC 6720: H2 formation on dust grains
• Dust Transport and Processing in Centrifugally Driven Protoplanetary Disk Winds
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• H_2 emission arises outside photodissociation regions in ultra-luminous infrared galaxies
• Jumping the Gap: The Formation Conditions and Mass Function of Pebble-Pile Planetesimals
• Effect of dust grain porosity on the appearance of protoplanetary disks
• Evolution of grain size distribution in high-redshift dusty quasars: Integrating large amounts of dust and unusual extinction curves
• High spatial resolution mid-infrared spectroscopy of NGC 5253: The stellar content of the embedded super-star cluster
• Predicting the stellar and non-equilibrium dust emission spectra of high-resolution simulated galaxies with DART-Ray
• G11.2-0.3: The Young Remnant of a Stripped-Envelope Supernova
• Accelerating Dust Temperature Calculations with Graphics Processing Units
• The PhotoDissociation Region Toolbox: Software and Models for Astrophysical Analysis
• Are the spiral arms in the MWC 758 protoplanetary disc driven by a companion inside the cavity?
• Free-free and H42alpha emission from the dusty starburst within NGC 4945 as observed by ALMA
• Can Reflection from Grains Diagnose the Albedo?
• Dust Abundance Variations in the Magellanic Clouds: Probing the Lifecycle of Metals with All-Sky Surveys
• Lyman `bump' galaxies - II. A possible signature of massive extremely metal-poor or metal-free stars in z=3.1 Ly-alpha emitters
• Investigating the interstellar dust through the Fe K-edge
• Spitzer observations of SN 2014J and properties of mid-IR emission in Type Ia supernovae
• Feedback-Driven Evolution of the Far-Infrared Spectral Energy Distributions of Luminous and Ultraluminous Infrared Galaxies
• X-ray Halos and Large Grains in the Diffuse Interstellar Medium
• Derivation of a large isotropic diffuse sky emission component at 1.25 and 2.2um from the COBE/DIRBE data
• ALMA observations of Lyman-alpha Blob 1: halo sub-structure illuminated from within
• A detailed framework to incorporate dust in hydrodynamical simulations
• Heliospheric modulation of the interstellar dust flow on to Earth
• The Light Echo Around Supernova 2003gd in Messier 74
• Polycyclic aromatic hydrocarbons in spatially resolved extragalactic star forming complexes
• Disk Masses at the end of the main accretion phase: CARMA Observations and Multi-Wavelength Modeling of Class I Protostars
• Influence of grain growth on CO2 ice spectroscopic profiles : Modelling for dense cores and disks
• Identifying Anticyclonic Vortex Features Produced by the Rossby Wave Instability in Protoplanetary Disks
• Photoevaporation and spatial variation of grain sizes in Orion 114-426
• A Joint Chandra and Swift View of the 2015 X-Ray Dust Scattering Echo of V404 Cygni
• Dust Attenuation in Hydrodynamic Simulations of Spiral Galaxies
• X-Ray Scattering by Nonspherical Grains. I. Oblate Spheroids
• A survey of infrared supernova remnants in the Large Magellanic Cloud
• Influence of the Environment on PAH Emission in Star-Forming Regions
• Tracing planet-induced structures in circumstellar disks using molecular lines
• JWST Observations of Young protoStars (JOYS): overview of program and early results
• HST Observations of SGR 0526-66: New Constraints on Accretion and Magnetar Models
• Perturbations of SNe Ia lightcurves, colors and spectral features by circumstellar dust
• A likely flyby of binary protostar Z CMa caught in action
• X-ray radiative transfer in full 3D with SKIRT
• CHANDRA Observations of the X-ray Halo around the Crab Nebula
• Observing planet-disk interaction in debris disks
• Planet formation via pebble accretion in externally photoevaporating discs
• Identification of new transitional disk candidates in Lupus with Herschel
• Amount of intergalactic dust: constraints from distant supernovae and thermal history of intergalactic medium
• Galactic distributions of carbon- and oxygen-rich AGB stars revealed by the AKARI mid-infrared all-sky survey
• Dust attenuation law in JWST galaxies at z = 7-8
• Lyα emission from galaxies in the Epoch of Reionization
• The IRX-$\beta$ relation of high-redshift galaxies
• Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
• Dusty Blastwaves of Two Young LMC Supernova Remnants: Constraints on Postshock Compression
• Diversity of Galaxy Dust Attenuation Curves Drives the Scatter in the IRX-beta Relation
• Dust Extinction of Gamma-ray Burst Host Galaxies: Identification of Two Classes?
• Simulating Star Clusters Across Cosmic Time: II. Escape Fraction of Ionizing Photons from Molecular Clouds
• Anomalously Steep Reddening Law in Quasars: An Exceptional Example Observed in IRAS14026+4341
• The Cosmic Evolution of the IMF Under the Jeans Conjecture with Implications for Bottom-Heavy Ellipticals
• The soft X-ray blast in the apparently sub-luminous GRB 031203
• The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. IV. Lupus Observed with MIPS
• H2, CO, and Dust Absorption through Cold Molecular Clouds
• Graphite Revisited
• Rapid Elimination of Small Dust Grains in Molecular Clouds
• JWST Observations of Young protoStars (JOYS): Linked accretion and ejection in a Class I protobinary system
• Quiescent low-mass galaxies observed by JWST in the Epoch of Reionization
• A redshift-dependent IRX-$\beta$ dust attenuation relation for TNG50 galaxies
• Spectropolarimetry of High Redshift Obscured and Red Quasars
• First direct detection of a polarized companion outside of a resolved circumbinary disk around CS Cha
• Nautilus multi-grain model: Importance of cosmic-ray-induced desorption in determining the chemical abundances in the ISM
• Constraining the dynamical importance of hot gas and radiation pressure in quasar outflows using emission line ratios
• Transition disk chemistry and future prospects with ALMA
• Discovery of a Light Echo from Supernova 2003gd
• FUSE Measurements of Far Ultraviolet Extinction. I. Galactic Sight Lines
• Time-Dependent, Multifluid, Magnetohydrodynamic Shock Waves with Grain Dynamics I. Formulation and Numerical Tests
• Dust emission in star-forming dwarf galaxies: General properties and the nature of the sub-mm excess
• Multiple paths of deuterium fractionation in protoplanetary disks
• The Distance and the near-IR extinction of the Monoceros Supernova Remnant
• Can Fluffy Dust Alleviate the "Subsolar" Interstellar Abundance Problem?
• The ALMA Lupus protoplanetary disk survey: evidence for compact gas disks and molecular rings from CN
• Synthetic observations of simulated pillars of creation
• Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency
• MgII in the JWST Era: a Probe of Lyman Continuum Escape?
• The EROS2 search for microlensing events towards the spiral arms: the complete seven season results
• First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
• Surface Diffusion of Carbon Atoms as a Driver of Interstellar Organic Chemistry
• When sticking influences H2 formation
• On the redshift distribution and physical properties of ACT-selected DSFGs
• A new census of dust and polycyclic aromatic hydrocarbons at z=0.7-2 with JWST MIRI
• Distances to the Supernova Remnants in the Inner Disk
• Spatial Distribution of Dust Grains within H II Regions
• Modeling the Infrared Interstellar Extinction
• High Precision Dynamical Masses of Pre-Main Sequence Stars with ALMA and Gaia
• Initial phases of massive star formation in high infrared extinction clouds. I. Physical parameters
• Dust-correlated cm-wavelength continuum emission on translucent clouds ζ Oph and LDN 1780
• Inferring the HII region escape fraction of ionizing photons from infrared emission lines in metal-poor star-forming dwarf galaxies
• What can we learn about protoplanetary disks from analysis of mid-infrared carbonaceous dust emission?
• The Diffuse Galactic Far-Ultraviolet Sky
• Molecular Hydrogen Formation on Low Temperature Surfaces in Temperature Programmed Desorption Experiments
• Observations and modeling of the dust emission from the H2-bright galaxy-wide shock in Stephan's Quintet
• Solving grain size inconsistency between ALMA polarization and VLA continuum in the Ophiuchus IRS 48 protoplanetary disk
• The temperature structure of dusty planetary nebulae
• A detailed study of the optical attenuation of gamma-ray bursts in the Swift era
• Modeling Grain Alignment by Radiative Torques and Hydrogen Formation Torques in Reflection Nebula
• The Optical/Near-Infrared Extinction Law In Highly Reddened Regions
• Verifying reddening and extinction for Gaia DR1 TGAS main sequence stars
• Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains
• Giant scattering cones in obscured quasars
• The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5
• Spectropolarimetry and Modeling of the Eclipsing T Tauri Star KH 15D
• Gas morphology and energetics at the surface of PDRs: new insights with Herschel observations of NGC 7023
• Velocity profiles of [CII], [CI], CO, and [OI] and physical conditions in four star-forming regions in the Large Magellanic Cloud
• Mid-Infrared Spectropolarimetric Constraints on the Core-Mantle Interstellar Dust Model
• An Interferometric View of H-MM1. I. Direct Observation of NH3 Depletion
• Ionization and Dust Charging in Protoplanetary Disks
• GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
• Clustered Star Formation in the Small Magellanic Cloud. A Spitzer/IRAC View of the Star-Forming Region NGC 602/N 90
• The Small Magellanic Cloud Investigation of Dust and Gas Evolution (SMIDGE): The Dust Extinction Curve from Red Clump Stars
• Radiative properties of the first galaxies: rapid transition between blue and red
• A Resolved Ring of Debris Dust Around the Solar Analog HD 107146
• The Star Formation in Radio Survey: 3 - 33 GHz Imaging of Nearby Galaxy Nuclei and Extranuclear Star-forming Regions
• Measurements of Diffuse Sky Emission Components in High Galactic Latitudes at 3.5 and 4.9 um Using DIRBE and WISE Data
• Probing the Interstellar Dust towards the Galactic Centre: Dust Scattering Halo around AX J1745.6-2901
• The cosmic carbon footprint of massive stars stripped in binary systems
• The Millimeter Continuum Size-Frequency Relationship in the UZ Tau E Disk
• Evidence for quasar fast outflows being accelerated at the scale of tens of parsecs
• Herschel photometric observations of the low metallicity dwarf galaxy NGC 1705
• Effects of dust scattering albedo and 2175 A bump on ultraviolet colours of normal disc galaxies
• X-ray Desorption of Molecules from Grains in Protoplanetary Disks
• Physical Dust Models for the Extinction toward Supernova 2014J in M82
• Measurements of the mean diffuse galactic light spectrum in the 0.95 μm to 1.65 μm band from CIBER
• Close-up view of a luminous star-forming galaxy at z=2.95
• CHANG-ES X: Spatially-resolved Separation of Thermal Contribution from Radio Continuum Emission in Edge-on Galaxies
• Numerical Simulations of Turbulent Molecular Clouds Regulated by Radiation Feedback Forces II: Radiation-Gas Interactions and Outflows
• Ly-alpha Radiative Transfer: Monte-Carlo Simulation of the Wouthuysen-Field Effect
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• Rocket Observations of Far-Ultraviolet Dust Scattering in NGC 2023
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Probing the Spatial Distribution of the Interstellar Dust Medium by High Angular Resolution X-ray Halos of Point Sources
• Simulated Galaxy Interactions as Probes of Merger Spectral Energy Distributions
• Resolved Multifrequency Radio Observations of GG Tau
• A Light Echo from Type Ia Supernova 1995E?
• Using the X-ray Dust Scattering Halo of 4U 1624-490 to determine distance and dust distributions
• Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
• Diversity of supernovae Ia determined using equivalent widths of Si II 4000
• A new hybrid radiative transfer method for massive star formation
• Temperature Profiles and the Effect of AGN on Submillimeter Emission from BLAST Observations of Resolved Galaxies
• The Spitzer c2d Survey of Nearby Dense Cores: Jet and Molecular Outflow Associated with a YSO in core A of L1251
• Properties of protostars in the Elephant Trunk globule IC 1396A
• VLT/X-shooter GRBs: Individual extinction curves of star-forming regions
• An Evolutionary Paradigm for Dusty Active Galaxies at Low Redshift
• Linking Characteristics of the Polycyclic Aromatic Hydrocarbon Population with Galaxy Properties: A Quantitative Approach Using the NASA Ames PAH IR Spectroscopic Database
• Simulations of polarized dust emission
• The population of Young Stellar Clusters throughout the disk of M33
• A wildly flickering jet in the black hole X-ray binary MAXI J1535-571
• A New Measurement of the Average FUV Extinction Curve
• The V1647 Ori (IRAS 05436-0007) Protostar and its Environment
• Time evolution of simple molecules during proto-star collapse
• Spitzer Observations of the Type Ia Supernova Remnant N103B: Kepler's Older Cousin?
• Panchromatic Spectral Energy Distributions of Dusty Galaxies with RADISHE. I. Predictions for Herschel: Correlating Colors with Galactic Energy Sources
• GIARPS High-resolution Observations of T Tauri stars (GHOsT). III. A pilot study of stellar and accretion properties
• Shiva: the dust destruction model
• Populations of Young Stellar Objects in Nearby Molecular Clouds
• Excitation and charge transfer in hydrogen-proton collisions at 5--80 keV and application to astrophysical shocks
• Supernova Remnants in the AKARI IRC Survey of the Large Magellanic Cloud
• Constraining the radial drift of millimeter-sized grains in the protoplanetary disks in Lupus
• Interplay of gas and ice during cloud evolution
• Some Stars are Totally Metal: A New Mechanism Driving Dust Across Star-Forming Clouds, and Consequences for Planets, Stars, and Galaxies
• On the origins of polarization holes in Bok globules
• Chandra observation of the TeV source HESS J1834-087
• Spitzer Observations of Cold Dust Galaxies
• Magnetic fields in circumstellar disks: The potential of Zeeman observations
• Dust entrainment in photoevaporative winds: The impact of X-rays
• The Near-Infrared Extinction Law in Regions of High Av
• Herschel limits on far-infrared emission from circumstellar dust around nearby Type Ia supernovae
• The mid-infrared extinction law in the darkest cores of the Pipe Nebula
• Asymmetry in the Outburst of SN 1987A Detected Using Light Echo Spectroscopy
• HERschel Observations of Edge-on Spirals (HEROES). IV. Dust energy balance problem
• Molecular Hydrogen in the Ionized Region of Planetary Nebulae
• The X-ray Halo of GX5-1
• Wall emission in circumbinary disks: the case of CoKu Tau/4
• Mapping the Planetary Wake in HD 163296 with Kinematics
• Modeling the effects of dust evolution on the SEDs of galaxies of different morphological type
• Modelling dust processing and the evolution of grain sizes in the ISM using the method of moments
• Investigation of dust attenuation and star formation activity in galaxies hosting GRBs
• Infrared Supernova Remnants and their Infrared to X-ray Flux Ratios
• Asteroseismic Study on Cluster Distance Moduli for RGB Stars in NGC 6791 and NGC 6819
• Warm gas towards young stellar objects in Corona Australis - Herschel/PACS observations from the DIGIT key programme
• The young protostellar disk in IRAS16293-2422 B is hot and shows signatures of gravitational instability
• Velocities of warm galactic outflows from synthetic Hα observations of star-forming galaxies
• Galactic foregrounds: Spatial fluctuations and a procedure of removal
• Modeling ionized gas in low-metallicity environments: the Local Group dwarf galaxy IC10
• The Dusty Heart of NGC 4151 Revealed by $\lambda \sim$1-40 $\mu$m Reverberation Mapping and Variability: A Challenge to Current Clumpy Torus Models
• Radiation feedback on dusty clouds during Seyfert activity
• Spirals, shadows & precession in HD 100453 -- I. The orbit of the binary
• A Massive Star is Born: How Feedback from Stellar Winds, Radiation Pressure, and Collimated Outflows Limits Accretion onto Massive Stars
• Observational studies on the Near-Infrared Unidentified Emission Bands in Galactic HII regions
• Confirmation of the VeLLO L1148-IRS: Star Formation at very low (Column) Density
• No Transition Disk? Infrared Excess, PAH, H2, and X-rays from the Weak-Lined T Tauri Star DoAr 21
• The impact of AGN-driven winds on physical and observable galaxy sizes
• Inferring (Sub)millimeter Dust Opacities and Temperature Structure in Edge-on Protostellar Disks From Resolved Multi-Wavelength Continuum Observations: The Case of the HH 212 Disk
• The Spitzer Survey of Interstellar Clouds in the Gould Belt. VI. The Auriga-California Molecular Cloud observed with IRAC and MIPS
• Complex organic molecules along the accretion flow in isolated and externally irradiated protoplanetary disks
• Sustained FU Orionis-type outbursts from colliding discs in stellar flybys
• X-ray versus Optical Observations of Active Galactic Nuclei: Evidence for Large Grains?
• Probing Cosmic Dawn: Modelling the Assembly History, SEDs, and Dust Content of Selected $z\sim 9$ Galaxies
• PDFchem: A new fast method to determine ISM properties and infer environmental parameters using probability distributions
• X-Ray Absorption and Scattering by Interstellar Grains
• Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations
• The Spitzer Survey of Interstellar Clouds in the Gould Belt. V. Ophiuchus North Observed with IRAC and MIPS
• Properties and alignment of interstellar dust grains toward Type Ia Supernovae with anomalous polarization curves
• An Echo of Supernova 2008bk
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Constraints on the structure of hot exozodiacal dust belts
• Thermal balance and comparison of gas and dust properties of dense clumps in the Hi-GAL survey
• Interstellar-Medium Mapping in M82 Through Light Echoes Around Supernova 2014J
• Deep JHKs and Spitzer Imaging of Four Isolated Molecular Cloud Cores
• The Impact of Feedback in Massive Star Formation. II. Lower Star Formation Efficiency at Lower Metallicity
• Evolution of the 1919 Ejecta of V605 Aquilae
• Diffuse Interstellar Bands and the Ultraviolet Extinction Curves: The Missing Link Revisited
• Thirty years of SN 1980K: Evidence for light echoes
• How chemistry influences cloud structure, star formation, and the IMF
• ALMA polarimetry measures magnetically aligned dust grains in the torus of NGC 1068
• GALEX UV properties of the polar ring galaxy MCG-05-07-001 and the shell galaxies NGC 1210 and NGC 5329
• The impact of astrophysical dust grains on the confinement of cosmic rays
• Si K Edge Structure and Variability in Galactic X-Ray Binaries
• Effect of MHD wind-driven disk evolution on the observed sizes of protoplanetary disks
• Dust Properties in the FUV in Ophiuchus
• ESO-H$\alpha$~574 and Par-Lup3-4 Jets: Exploring the spectral, kinematical and physical properties
• Testing Mass Loss in Large Magellanic Cloud Cepheids using Infrared and Optical Observations
• Far-ultraviolet fluorescent molecular hydrogen emission map of the Milky Way Galaxy
• Surrogate modelling the Baryonic Universe I: The colour of star formation
• Simulating the atomic and molecular content of molecular clouds using probability distributions of physical parameters
• LOC program for line radiative transfer
• Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
• Identification of tidal features in deep optical galaxy images with Convolutional Neural Networks
• SHARDS: stellar populations and star formation histories of a mass-selected sample of 0.65<z<1.1 galaxies
• The Carnegie Supernova Project I: methods to estimate host-galaxy reddening of stripped-envelope supernovae
• Polarizing efficiency as a guide of grain growth and interstellar magnetic field properties
• The X-ray dust scattered rings of the black hole low mass binary V404 Cyg
• On the importance of scattering at 8 microns: Brighter than you think
• Constraint on intergalactic dust from thermal history of intergalactic medium
• Large-scale Vortices in Protoplanetary Disks: On the observability of possible early stages of planet formation
• The origin of the late-time luminosity of supernova 2011dh
• Herschel survey of brown dwarf disks in Rho Ophiuchi
• Clustering and dynamic decoupling of dust grains in turbulent molecular clouds
• The average dust attenuation curve at z~1.3 based on HST grism surveys
• Rotational Desorption of Ice Mantles and Complex Molecules from Suprathermally Rotating Dust Grains around Young Stellar Objects
• Ring formation by coagulation of dust aggregates in early phase of disk evolution around a protostar
• Aperture Synthesis Imaging of V892 Tau and PV Cep: Disk Evolution
• Measurement of the Oxidation state of Fe in the ISM using X-ray Absorption Spectroscopy
• GW Ori: circumtriple rings and planets
• Chandra observations of the elusive pulsar wind nebula around PSR B0656+14
• An extremely low mid-infrared extinction law toward the Galactic Center and 4% distance precision to 55 classical Cepheids
• Modelling galaxy spectra in presence of interstellar dust. II. From the UV to the far infrared
• Interstellar extinction and polarization -- A spheroidal dust grain approach perspective
• Bow shocks, bow waves, and dust waves. I. Strong coupling limit
• Fast methods for tracking grain coagulation and ionization. I. Analytic derivation
• Uncovering Red and Dusty Ultraluminous X-ray Sources with Spitzer
• From large scale gas compression to cluster formation in the Antennae overlap region
• Probing the cold magnetized Universe with SPICA-POL (B-BOP)
• Thick turbulent gas disks with magnetocentrifugal winds in active galactic nuclei - Model infrared emission and optical polarization
• A multiwavelength study of the Magellanic-type galaxy NGC 4449 - I. Modelling the spectral energy distribution, the ionization structure and the star formation history
• Millimeter and Submillimeter Excess Emission in M33 revealed by Planck and LABOCA
• Super-Eddington mass growth of intermediate-mass black holes embedded in dusty circumnuclear disks
• A systematic study of radiative torque grain alignment in the diffuse interstellar medium
• Heavy dust obscuration of z=7 galaxies in a cosmological hydrodynamic simulation
• Resolved Star Formation on Sub-galactic Scales in a Merger at z=1.7
• WISE Detection of the Galactic Low-Mass X-Ray Binaries
• Dust Destruction by Charging: A Possible Origin of Grey Extinction Curves of Active Galactic Nuclei
• The relationship between X-ray and optical absorbers in active galactic nuclei
• Dissection of Halpha Emitters : Low-z Analogs of z>4 Star-Forming Galaxies
• Earliest phases of star formation (EPoS): Dust temperature distributions in isolated starless cores
• Shattering by turbulence as a production source of very small grains
• Interstellar Extinction by Spheroidal Dust Grains
• Formation and properties of astrophysical carbonaceous dust. I: ab-initio calculations of the configuration and binding energies of small carbon clusters
• X-ray Dust Scattering at Small Angles: The Complete Halo around GX13+1
• Modelling interstellar extinction and polarization with spheroidal grains
• Interstellar dust along the line of sight of GX 3+1
• Ultraviolet Halos Around Spiral Galaxies. I. Morphology
• Evolution of dust grain size distribution by shattering in the interstellar medium: robustness and uncertainty
• Spitzer observations of supernova remnants: II. Physical conditions and comparison with HH7 and HH54
• Observing dust settling and coagulation in circumstellar discs: Selected constraints from high resolution imaging
• HerMES: Herschel-SPIRE observations of Lyman Break Galaxies
• The sweeping rate in diffusion-mediated reactions on dust grain surfaces
• Comparison of the Diffuse Halpha and FUV Continuum Backgrounds: On the Origins of the Diffuse Halpha Background
• Evidence that Shocks Destroy Small PAH Molecules in Low-luminosity Active Galactic Nuclei
• Integrated parameters of star clusters: A comparison of theory and observations
• LABOCA observations of giant molecular clouds in the south west region of the Small Magellanic Cloud
• Detection of the Intermediate-width Emission Line Region in Quasar OI 287 with the Broad Emission Line Region Obscured by the Dusty Torus
• The Spitzer Survey of Interstellar Clouds in the Gould Belt. IV. Lupus V and VI Observed with IRAC and MIPS
• Infrared Spectroscopy of Halos of Edge-on Galaxies
• Imaging Polarization of the Blue-Excess Hot Dust-Obscured Galaxy WISE J011601.41-050504.0
• The PDR structure and kinematics around the compact HII regions S235A and S235C with [CII], [13CII], [OI] and HCO+ line profiles
• Light Echoes of Transients and Variables in the Local Universe
• On the Interpretation of Far-infrared Spectral Energy Distributions. I: The 850 $\mu$m Molecular Mass Estimator
• LABOCA mapping of the infrared dark cloud MSXDC G304.74+01.32
• The Highly Dynamic Behavior of the Innermost Dust and Gas in the Transition Disk Variable LRLL 31
• On the origin of low escape fractions of ionizing radiation from massive star-forming galaxies at high redshift
• Far-ultraviolet Observations of the Taurus-Perseus-Auriga Complex
• Meso-scale Instability Triggered by Dust Feedback in Dusty Rings: Origin and Observational Implications
• Estimating dust distances to Type Ia supernovae from colour excess time-evolution
• Dust properties of Lyman break galaxies in cosmological simulations
• The impact of freeze-out on collapsing molecular clouds
• CO2-rich protoplanetary discs as a probe of dust radial drift & trapping
• Magnification of Photometric LRGs by Foreground LRGs and Clusters in SDSS
• The Spitzer c2d Survey of Nearby Dense Cores: III: Low Mass Star Formation in a Small Group, L1251B
• An embedded active nucleus in the OH megamaser galaxy IRAS16399-0937
• Composite Interstellar Grains
• The JCMT Gould Belt Survey: the effect of molecular contamination in SCUBA-2 observations of Orion A
• The Ultraviolet Extinction Map and Dust Property at High Galactic Latitude
• Radiative transfer of ionizing radiation through gas and dust: stellar source case
• Contribution of polycyclic aromatic hydrocarbon ionization to neutral gas heating in galaxies: model versus observations
• Near-Infrared Detection of a Super-Thin Disk in NGC 891
• Determination of the far-infrared dust opacity in a prestellar core
• New constraints on the dust and gas distribution in the LkCa 15 disk from ALMA
• The impact of cosmic-ray attenuation on the carbon cycle emission in molecular clouds
• Results from DROXO. II. - [Ne II] and X-ray emission from Rho Ophiuchi young stellar objects
• Differences between CO- and calcium triplet-derived velocity dispersions in spiral galaxies: evidence for central star formation?
• The chemical signature of surviving Population III stars in the Milky Way
• Infrared study of transitional disks in Ophiuchus with Herschel
• Dynamics during outburst: VLTI observations of the young eruptive star V1647 Ori during its 2003-2006 outburst
• Extended X-ray emission in the vicinity of the microquasar LS 5039: pulsar wind nebula?
• Evolution of young protoclusters embedded in dense massive clumps. A new grid of population synthesis SED models and a new set of L/M evolutionary tracks
• A Framework for Modeling Polycyclic Aromatic Hydrocarbon Emission in Galaxy Evolution Simulations
• The co-evolution of molecular hydrogen and the grain size distribution in an isolated galaxy
• Extinction and dust properties in a clumpy medium
• The structured environments of embedded star-forming cores. PACS and SPIRE mapping of the enigmatic outflow source UYSO 1
• Dust charge distribution in the interstellar medium
• On Buckyonions as an Interstellar Grain Component
• The X-ray Halo of Cen X-3
• Extinction in the 11.2 micron PAH band and the low L_11.2/L_IR in ULIRGs
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• Dust evolution with MUPPI in cosmological volumes
• Dust growth, fragmentation and self-induced dust traps in PHANTOM
• IGM Transmission Bias for $z$ $\ge$ 2.9 Lyman Continuum Detected Galaxies
• On the stickiness of CO${}_2$ and H${}_2$O ice particles
• DART-Ray: a 3D ray-tracing radiative transfer code for calculating the propagation of light in dusty galaxies
• Isentropic thermal instability in atomic surface layers of photodissociation regions
• Interstellar Silicon Depletion and the Ultraviolet Extinction
• Effects of grain growth on the interstellar polarization curve
• Optical/near-infrared observations of the Fried Egg Nebula: Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant
• SOFIA/HAWC+ traces the magnetic fields in NGC 1068
• Comparison of cosmological simulations and deep submillimetre galaxy surveys
• The highly polarized dusty emission core of Cygnus A
• Impact of distance determinations on Galactic structure. I. Young and intermediate-age tracers
• Mid-infrared imaging- and spectro-polarimetric subarcsecond observations of NGC 1068
• Determining Type Ia Supernovae Host galaxy extinction probabilities and a statistical approach to estimating the absorption-to-reddening ratio $R_V$
• Grain Destruction in a Supernova Remnant Shock Wave
• Predicting sub-millimeter flux densities from global galaxy properties
• Systematic biases in determining dust attenuation curves through galaxy SED fitting
• The role of OH in the chemical evolution of protoplanetary disks. I. The comet-forming region
• The implications of dust for high-redshift protogalaxies and the formation of binary disks
• Effect of grain size distribution and size-dependent grain heating on molecular abundances in starless and pre-stellar cores
• Lyman-alpha radiative transfer: Modeling spectrum and surface brightness profile of Lyman-alpha emitting galaxies at z=3-6
• AKARI's infrared view on nearby stars : Using AKARI Infrared Camera All-Sky Survey, 2MASS, and Hipparcos catalog
• Extended Red Emission in IC59 and IC63
• On Graphene in the Interstellar Medium
• Observational signatures of linear warps in circumbinary discs
• Dust grain dynamics in C-Type shock waves in molecular clouds
• Empirical determination of Einstein A-coefficient ratios of bright [Fe II] lines
• A bimodal dust grain distribution in the IC 434 HII region
• Dust masses and star formation in bright IRAS galaxies Application of a physical model for the interpretation of FIR observations
• Modeling Spitzer observations of VV Ser. II. an extended quantum heated nebula and a disk shadow
• A Chandra search for the pulsar wind nebula around PSR B1055-52
• Spitzer Imaging and Spectral Mapping of the Oxygen-Rich Supernova Remnant G292.0+1.8
• Dissecting the different components of the modest accretion bursts of the very young protostar HOPS 373
• Physical and chemical modeling of the starless core L1512
• Dust evolution across the Horsehead Nebula
• Revisiting Attenuation Curves: the Case of NGC 3351
• Origin and evolution of dust-obscured galaxies in galaxy mergers
• The First Reported Infrared Emission from the SN 1006 Remnant
• Derivation of an Analytical Approximation of the Spectrum of Spinning Dust Emission
• AKARI's infrared view on nearby stars : Using AKARI Infrared Camera All-Sky Survey, 2MASS, and Hipparcos catalog
• Interstellar Extinction
• Uncovering the Spectral Energy Distribution in Active Galaxies Using High Ionization Mid-infrared Emission Lines
• Integral Field Spectroscopy of Balmer-Dominated Shocks in the Magellanic Cloud Supernova Remnant N103B
• Interstellar Grains -- The 75th Anniversary
• Tracing the [FeII]/[NeII] ratio and its relationship with other ISM indicators within star forming dwarf galaxies: a Spitzer IRS archival study
• Ray-tracing simulations and spectral models of X-ray radiation in dusty media
• The role of carbon grains in the deuteration of H2
• Unshifted Metastable He I* Mini-Broad Absorption Line System in the Narrow Line Type 1 Quasar SDSS J080248.18$+$551328.9
• Determining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry
• The Dust Scattering Halo of Cygnus X-3
• FAUST IX. Multi-band, multi-scale dust study of L1527 IRS. Evidence for dust properties variations within the envelope of a Class 0/I YSO
• Identifying Young Stellar Objects in the Outer Galaxy: l = 224 deg Region in Canis Major
• Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud
• Candidate Water Vapor Lines to Locate the ${\mathrm{H}}_2\mathrm{O}$ Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter ${\mathrm{H}}_2$${}^{16}\mathrm{O}$ and ${\mathrm{H}}_2$${}^{18}\mathrm{O}$ Lines
• Rocket and FUSE Observations of IC 405: Differential Extinction and Fluorescent Molecular Hydrogen
• Feeding the Accretion Disk from the Dusty Torus in a Reddened Quasar
• Probing interstellar extinction near the 30 Doradus nebula with red giant stars
• Disk Masses and Dust Evolution of Protoplanetary Disks Around Brown Dwarfs
• Shaping the structure of a GMC with radiation and winds
• A multiwavelength analysis of planetary nebulae in the Large Magellanic Cloud
• X-Shooter spectroscopy of young stellar objects - VI - HI line decrements
• Sub-Arcsecond Mid-Infrared Observations of NGC 6240: Limitations of AGN-Starburst Power Diagnostics
• Near-IR search for lensed supernovae behind galaxy clusters: I. Observations and transient detection efficiency
• Detection of Anomalous Microwave Emission in the Pleiades Reflection Nebula with WMAP and the COSMOSOMAS Experiment
• A controlled study of cold dust content in galaxies from $z=0-2$
• X-ray Scattering Halos from the Galactic Center: Implications for Diffuse Emission Around SgrA*
• Studying the Physical Properties of Tidal Features I. Extracting Morphological Substructure in CANDELS Observations and VELA Simulations
• The edge-on protoplanetary disk HH 48 NE I. Modeling the geometry and stellar parameters
• Comparison of the extraplanar H$\alpha$ and UV emissions in the halos of nearby edge-on spiral galaxies
• Balmer breaks in simulated galaxies at z>6
• The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
• Delayed Photons from Binary Evolution Help Reionize the Universe
• A New Technique for Measuring Polycyclic Aromatic Hydrocarbon Emission in Different Environments
• The KOSMA-$\tau$ PDR Model -- I. Recent updates to the numerical model of photo-dissociated regions
• Deep, ultra-high-resolution radio imaging of submillimetre galaxies using Very Long Baseline Interferometry
• On the missing 2175 Angstroem-bump in the Calzetti extinction curve
• Interstellar Extinction and Elemental Abundances
• Dust Scattering and the Radiation Pressure Force in the M82 Superwind
• The Magnetic Field Across the Molecular Warped Disk of Centaurus A
• Radiation fields in star-forming galaxies: the disk, thin disk and bulge
• Far-Infrared Spectral Energy Distributions and Photometric Redshifts of Dusty Galaxies
• Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
• The standard model of low-mass star formation applied to massive stars: multi-wavelength modelling of IRAS 20126+4104
• ROBO: a Model and a Code for the Study of the Interstellar Medium
• The hot core-ultracompact HII connection in G10.47+0.03
• Ionizing photon production and escape fractions during cosmic reionization in the TNG50 simulation
• Ultraviolet Radiative Transfer Modeling of Nearby Galaxies with Extraplanar Dusts
• Different degrees of nitrogen and carbon depletion in the warm molecular layers of protoplanetary disks
• From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?
• Radiation hydrodynamics including irradiation and adaptive mesh refinement with AZEuS. I. Methods
• Large Interstellar Polarisation Survey II. UV/optical study of cloud-to-cloud variations of dust in the diffuse ISM
• Higher prevalence of X-ray selected AGN in intermediate age galaxies up to z~1
• Chemical signatures of a warped protoplanetary disc
• The Dust Scattering Model Can Not Explain The Shallow X-ray Decay in GRB Afterglows
• Unbiased Monte Carlo continuum radiative transfer in optically thick regions
• [CII] $158\mu \mathrm{m}$ line emission from Orion A. I. A template for extragalactic studies?
• Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
• ASTE observations in the 345 GHz window towards the HII region N113 of the Large Magellanic Cloud
• Dust dynamics in RAMSES -- I. Methods and turbulent acceleration
• A survey of T Tauri stars with AKARI toward the Taurus-Auriga region
• Impact of PAH photodissociation on the formation of small hydrocarbons in the Orion Bar and the Horsehead PDRs
• Kinematic evidence for an embedded planet in the IM Lupi disc
• Dust evolution processes constrained by extinction curves in nearby galaxies
• Quantitative polarimetry of the disk around HD 169142
• The Fate of AGB Wind in Massive Galaxies and the ICM
• The dust SED of dwarf galaxies I. The case of NGC 4214
• The Spectral Energy Distributions of Red 2MASS AGN
• Photoelectric heating and [CII] cooling in translucent clouds: results for cloud models based on simulations of compressible MHD turbulence
• Planet gap opening across stellar masses
• Interpreting Brightness Asymmetries in Transition Disks: Vortex at Dead Zone or Planet Carved Gap Edges?
• Using cm Observations to Constrain the Abundance of Very Small Dust Grains in Galactic Cold Cores
• IRAS 20050+2720: Anatomy of a young stellar cluster
• Anatomy of A Dark Burst - The Afterglow of GRB 060108
• Role of Thermal and Non-thermal Processes in the ISM of Magellanic Clouds
• Physical conditions in three high-z H2-bearing DLAs: implications for grain size
• Spitzer observations of a 24 micron shadow: Bok Globule CB190
• Young, UV-bright Stars Dominate Dust Heating in Star Forming Galaxies
• Dust grains cannot grow to millimeter sizes in protostellar envelopes
• The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
• The power of the rings: the GRB 221009A soft X-ray emission from its dust-scattering halo
• Observing the gas component of circumplanetary disks around wide-orbit planet-mass companions in the (sub)mm regime
• Spatial and Temporal Variations in Interstellar Absorption toward HD 72127AB
• VISION - Vienna Survey in Orion II. Infrared extinction in Orion A
• Spectropolarimetry of the 3.4 micron absorption feature in NGC 1068
• Serendipitous Discovery of An Infrared Bow Shock Near PSR J1549-4848 with Spitzer
• Circumnuclear Star Clusters in the Galaxy Merger NGC 6240, Observed with Keck Adaptive Optics and HST
• The Origin of the Doppler-flip in HD 100546: a large scale spiral arm generated by an inner binary companion
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Hubble Space Telescope NICMOS Polarization Observations of Three Edge-on Massive YSOs
• Dark dust II: Properties in the general field of the diffuse ISM
• The extinction law for molecular clouds. Case study of B 335
• Dust-free starburst galaxies at redshifts $z>10$
• Modelling methanol and hydride formation in the JWST Ice Age era
• The Widespread Presence of Nanometer-size Dust Grains in the Interstellar Medium of Galaxies
• Single-Star HII Regions as a Probe of Massive Star Spectral Energy Distributions
• Benchmarking Dust Emission Models in M101
• Spinning dust radiation: a review of the theory
• Optical and infrared emission of H II complexes as a clue to the PAH life cycle
• Tracing the Magnetic Field of IRDC G028.23$-$00.19 Using NIR Polarimetry
• Evidence from SOFIA Imaging of Polycyclic Aromatic Hydrocarbon Formation along a Recent Outflow in NGC 7027
• On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation. II. The Effect of Metallicity
• Over-sized gas clumps in an extremely-metal-poor molecular cloud revealed by ALMA's pc-scale maps
• Dust attenuation in the restframe ultraviolet: constraints from star-forming galaxies at z~1
• Bow shocks, bow waves, and dust waves. II. Beyond the rip point
• Modelling the evolution of PAH abundance in galaxies
• Simulations Find Our Accounting of Dust-Obscured Star Formation May Be Incomplete
• The disk of FU Orionis viewed with MATISSE/VLTI: first interferometric observations in $L$ and $M$ bands
• Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
• The isotropic interplanetary dust cloud and near-infrared extragalactic background light observed with COBE/DIRBE
• Infrared Properties of z=7 Galaxies from Cosmological Simulations
• The dust attenuation law in $z\sim 6$ quasars
• (Sub)millimeter Dust Polarization of Protoplanetary Disks from Scattering by Large Millimeter-Sized Irregular Grains
• Toward understanding physical origin of 2175Å extinction bump in interstellar medium
• Polycyclic Aromatic Hydrocarbon Emission in the Central Regions of Three Seyferts the Implication for Underlying Feedback Mechanisms
• Interstellar Silicate Dust in the z=0.89 Absorber Towards PKS 1830-211: Crystalline Silicates at High Redshift?
• A molecular cloud within the light echo of V838 Monocerotis
• AKARI Near-infrared Spectral Observations of Shocked H2 Gas of the Supernova Remnant IC 443
• How Much Graphene in Space?
• Enhanced H2O formation through dust grain chemistry in X-ray exposed environments
• Probing the eccentricity in protostellar discs -- Modeling kinematics and morphologies
• Dusty Planetary Systems
• The circumstellar disk of FS Tau B - A self-consistent model based on observations in the mid-infrared with NACO -
• Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models
• AKARI Detection of the Infrared-Bright Supernova Remnant B0104-72.3 in the Small Magellanic Cloud
• Distribution of dust clouds around the central engine of NGC 1068
• Modelling CH${}_3$OH masers: Sobolev approximation and accelerated lambda iteration method
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Interferometric study on the temporal variability of the brightness distributions of protoplanetary disks
• EXORCISM: a spectroscopic survey of young eruptive variables (EXor and candidates)
• Outward Motion of Porous Dust Aggregates by Stellar Radiation Pressure in Protoplanetary Disks
• Late-Time Dust Emission from the Type IIn Supernova 1995N
• Bow shocks, bow waves, and dust waves. III. Diagnostics
• Non-equilibrium ionisation and radiative transport in an evolving supernova remnant
• Estimating reddening of the continuum and broad-line region of active galactic nuclei: the mean reddening of NGC 5548 and the size of the accretion disc
• Evolution of dust porosity through coagulation and shattering in the interstellar medium
• Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim 1.4$
• Far-Ultraviolet Observations of the Spica Nebula and the Interaction Zone
• Dust diffusion in SPH simulations of an isolated galaxy
• Self-scattering in protoplanetary disks with dust settling
• Dust-depletion sequences in damped Ly-α absorbers II. The composition of cosmic dust, from low-metallicity systems to the Galaxy
• An Investigation of the Dust Content in the Galaxy pair NGC 1512/1510 from Near-Infrared to Millimeter Wavelengths
• Probing the Innermost Ejecta Layers in SNR Kes 75: Implications for the Supernova Progenitor
• Chemical evolution of the gas in C-type shocks in dark clouds
• Effects of X-ray irradiation and disk flaring on the [NeII] 12.8 micron emission from young stellar objects
• Searching for planetary-mass T-dwarfs in the core of Serpens
• On the discrepancy between asteroseismic and Gaia DR1 TGAS parallaxes
• Simulated JWST datasets for multispectral and hyperspectral image fusion
• Cooling timescale of dust tori in dying active galactic nuclei
• Dust destruction in non-radiative shocks
• Spitzer Spectroscopy of the Galactic Supernova Remnant G292.0+1.8: Structure and Composition of the Oxygen-Rich Ejecta
• Evidence for Decay of Turbulence by MHD Shocks in Molecular Clouds via CO Emission
• Exploring Active Galactic Nuclei and Little Red Dots with the Obelisk simulation
• The accretion burst of the massive young stellar object G323.46 -0.08
• Dust abundance and grain size in galaxy halos
• Ly-alpha Radiative Transfer: A Stokes Vector Approach to Ly-alpha Polarization
• A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy
• On the Unusual Depletions toward Sk 155, or What Are the Small Magellanic Cloud Dust Grains Made of?
• Dust Evolution in the Dwarf Galaxy Holmberg II
• Insights from Synthetic Star-forming Regions: I. Reliable Mock Observations from SPH Simulations
• Interplay of dust alignment, grain growth and magnetic fields in polarization: lessons from the emission-to-extinction ratio
• The Mechanical Alignment of Dust (MAD) I: On the spin-up process of fractal grains by a gas-dust drift
• The Origin and Evolution of Lyman-alpha Blobs in Cosmological Galaxy Formation Simulations
• Infrared Studies of Molecular Shocks in the Supernova Remnant HB21: I. Thermal Admixture of Shocked H_2 Gas in the North
• Measuring the Heating and Cooling of the Interstellar Medium at High redshift: PAH and [C II] Observations of the Same Star Forming Galaxies at z~2
• 3D radiative transfer of intrinsically polarized dust emission based on aligned aspherical grains
• Lyman-$\alpha$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
• Spectral Softening in X-ray Afterglow of GRB 130925A as Predicted by Dust Scattering Model
• Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse
• Polycyclic Aromatic Hydrocarbon emission model in photodissociation regions I: Application to the 3.3, 6.2, and 11.2 $\mu$m bands
• Expected dust grain size distributions in galaxies detected by ALMA at $z>7$
• Modeling the Infrared Reverberation Response of the Circumnuclear Dusty Torus in AGNs: An Investigation of Torus Response Functions
• GG Tau A: Dark shadows on the ringworld
• Star formation and dust obscuration in the tidally distorted galaxy NGC 2442
• Disentangling protoplanetary disk gas mass and carbon depletion through combined atomic and molecular tracers
• UVIT observations of the Small Magellanic Cloud: Point source catalogue
• MIRIS observation of near-infrared diffuse Galactic light
• SDSS J163459.82+204936.0: A Ringed Infrared-Luminous Quasar with Outflows in both Absorption and Emission Lines
• Spectropolarimetry of Galactic stars with anomalous extinction sightlines
• The Physical Structure of Protoplanetary Disks: the Serpens Cluster Compared with Other Regions
• A kinematic excess in the annular gap and gas depleted cavity in the disc around HD 169142
• A faint companion around CrA-9: protoplanet or obscured binary?
• Modeling the Infrared Extinction toward the Galactic Center
• Estimators of Bolometric Luminosity and Black Hole Mass with Mid-infrared Continuum Luminosities for Dust-obscured Quasars: Prevalence of Dust-obscured SDSS Quasars
• Mapping Circumstellar Matter with Polarized Light - The Case of Supernova 2014J in M82
• YSO jets in the Galactic Plane from UWISH2: V - Jets and Outflows in M17
• Dust in the Wind with Resonant Drag Instabilities: I. The Dynamics of Dust-Driven Outflows in GMCs and HII Regions
• On the Simultaneous Modelling of Dust and Stellar Populations for Interpretation of Galaxy Properties
• A High Mass Dusty Disk Candidate: The Case of IRAS 18151-1208
• Chemical tracers of a highly eccentric AGB-main sequence star binary
• Ionisation feedback in star formation simulations: The role of diffuse fields
• Thermal fluctuations and nanoscale effects in the nucleation of carbonaceous dust grains
• Radiation-pressure-driven dust transport to galaxy halos at $z\sim 10$
• The red halos of SDSS low surface brightness disk galaxies
• A radiative transfer model for the spiral galaxy M33
• Spitzer Mid-infrared Upper Limits on Anomalous X-Ray Pulsars 1E 1048.1-5937, 1RXS J170849-400910, and XTE J1810-197
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. II. Features of Attenuation Law
• Linking the dust and chemical evolution: Taurus and Perseus -- New collisional rates for HCN, HNC, and their C, N, and H isotopologues
• Polarized Mid-Infrared Synchrotron Emission in the Core of Cygnus A
• ALMA observations of super-early galaxies: attenuation-free model predictions
• Dust Budget Crisis in Little Red Dots
• Breaking Orion's Veil bubble with fossil outflows
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• Molecular and Ionized Hydrogen in 30 Doradus. I. Imaging Observations
• Interstellar chemical differentiation across grain sizes
• Computational modeling of the class I low-mass protostar Elias 29 applying optical constants of ices processed by high energy cosmic ray analogs
• A multi-wavelength interferometric study of the massive young stellar object IRAS 13481-6124
• Dust and dark Gamma-Ray Bursts: mutual implications
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• Detection of Near-Infrared Water Ice at the Surface of the (pre)Transitional Disk of AB Aur: Informing Icy Grain Abundance, Composition, and Size
• Fractal dimension of optical cirrus in Stripe82
• Raman mapping of photodissociation regions
• Measurement of Dust Optical Properties in Coalsack
• Proper Plasma Analysis Practice (PPAP), an Integrated Procedure of the Extinction Correction and Plasma Diagnostics: a Demo with an HST/WFC3 Image Set of NGC6720
• Kinematic and thermal signatures of the directly imaged protoplanet candidate around Elias 2-24
• Extinction Law at a Distance up to 25 kpc toward the Galactic Poles
• Dust Survival in Galactic Winds
• Spread of the dust temperature distribution in circumstellar disks
• ERGO-ML: Comparing IllustrisTNG and HSC galaxy images via contrastive learning
• Joint Modelling of Dust Scattering and Thermal Emission: The Spider Complex
• AFGL 5180 and AFGL 6366S: sites of hub-filament systems at the opposite edges of a filamentary cloud
• Dust attenuation in galaxies at cosmic dawn from the FirstLight simulations
• G048.66-0.29: Physical State of an Isolated Site of Massive Star Formation
• Efficiency of the top-down PAH-to-fullerene conversion in UV irradiated environments
• Is the star formation rate in $z\sim 6$ quasars overestimated?
• The evolution of circumstellar discs in the Galactic Centre: an application to the G-clouds
• Characteristics of small protoplanetary disc warps in kinematic observations
• Ice mantles on dust grains: dramatic variation of thickness with grain size
• Lyman-alpha radiation pressure: an analytical exploration
• Young stellar clusters and associations in M33
• Detection of Polarized Infrared Emission by Polycyclic Aromatic Hydrocarbons in the MWC 1080 Nebula
• Constraints on the Progenitor of SN 2010jl and Pre-Existing Hot Dust in its Surrounding Medium
• Oxygen in dense interstellar gas - the oxygen abundance of the star forming core rho Oph A
• UV-Luminous, Star-Forming Hosts of z~2 Reddened Quasars in the Dark Energy Survey
• Gas absorption and dust extinction towards the Orion Nebula Cluster
• Properties of interstellar dust responsible for extinction laws with unusually low total-to-selective extinction ratios of Rv=1-2
• The contribution of globular clusters to cosmic reionization
• Far-infrared dust properties in the Galaxy and the Magellanic Clouds
• Resolved spectral variations of the centimetre-wavelength continuum from the rho Oph W photo-dissociation-region
• Structures in circumbinary disks: Prospects for observability
• VLTI-MATISSE L- and N-band aperture-synthesis imaging of the unclassified B[e] star FS Canis Majoris
• Dust Extinction Law in Nearby Star-Resolved Galaxies. I. M31 Traced by Supergiants
• Interstellar Extinction and Elemental Abundances: Individual Sight Lines
• The cosmic transparency measured with Type Ia supernovae: implications for intergalactic dust
• Interstellar Silicate Dust in the z=0.685 Absorber Toward TXS 0218+357
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• 3D structure of HII region Sh2-235 from tunable-filter optical observations
• Dwarf satellites of high-z Lyman Break Galaxies: a free lunch for JWST
• The infrared-luminous progenitors of high-z quasars
• Dust Extinction Law in Nearby Star-Resolved Galaxies. II. M33 Traced by Supergiants
• Galactic Latitude Dependence of Near-Infrared Diffuse Galactic Light : Thermal Emission or Scattered Light?
• Revisiting the lifetime estimate of large presolar grains in the interstellar medium
• Cold dust clumps in dynamically hot gas
• Globules and pillars in Cygnus X III. Herschel and upGREAT/SOFIA far-infrared spectroscopy of the globule IRAS 20319+3958 inCygnus X
• Synthetic observations of spiral arm tracers of a simulated Milky Way analog
• Accretion-ejection connection in the young brown dwarf candidate ISO-Cha1 217
• Mid-infrared extinction and fresh silicate dust towards the Galactic Center
• Effects of dust evolution on the abundances of CO and H${}_2$
• Systematic Error of the Gaia DR1 TGAS Parallaxes from Data for the Red Giant Clump
• Systematic errors in dust mass determinations: Insights from laboratory opacity measurements
• The role of grain size in AGN torus dust models
• Dust accretion and destruction in galaxy groups and clusters
• Molecular Gas in Intermediate Redshift ULIRGs
• High contrast and resolution near infrared photometry of the core of R136
• Dynamics of dust grains in turbulent molecular clouds. Conditions for decoupling and limits of different numerical implementations
• Dusty plasma in active galactic nuclei
• The Kuiper Belt and Other Debris Disks
• IR characteristic emission and dust properties of star-forming galaxies at 4.5 $<$ z $<$ 6.2
• On the Impact of Inclination-Dependent Attenuation on Derived Star Formation Histories: Results from Disk Galaxies in the Great Observatories Origins Deep Survey Fields
• Feasibility of detecting and characterizing embedded low-mass giant planets in gaps in the VIS/NIR wavelength range
• SIMBA's view of the epsilon Eri disk
• Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems
• Probing the 9.7μm Interstellar Silicate Extinction Profile through the Spitzer/IRS Spectroscopy of OB Stars
• AKARI near- and mid-infrared spectroscopy of APM 08279+5255 at z=3.91
• Gap Opening and Inner Disk Structure in the Strongly Accreting Transition Disk of DM Tau
• X-Shooter spectroscopy of FU Tau A
• Synthesized grain size distribution in the interstellar medium
• CO Multi-line Imaging of Nearby Galaxies (COMING). XII. CO-to-H${}_2$ Conversion Factor and Dust-to-Gas Ratio
• Classification Study of WISE Infrared Sources: Identification of Candidate Asymptotic Giant Branch Stars
• Marginal likelihoods of distances and extinctions to stars: computation and compact representation
• The Age-Dependence of Mid-Infrared Emission Around Young Star Clusters
• A resolved and asymmetric ring of PAHs within the young circumstellar disk of IRS 48
• Mass loss rates from mid-IR excesses in LMC and SMC O stars
• Light echo of V838 Monocerotis: properties of the echoing medium
• The JCMT BISTRO Survey: Multi-wavelength polarimetry of bright regions in NGC 2071 in the far-infrared/submillimetre range, with POL-2 and HAWC+
• Cygnus X-3's Little Friend
• Infrared view of the multiphase ISM in NGC 253 I. Observations and fundamental parameters of the ionised gas
• Local Analogs to High-Redshift Galaxies: I. Characterization of Dust Emission and Star Formation History
• On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump
• Linking ice and gas in the Lambda Orionis Barnard 35A cloud
• Measuring the Local ISM along the Sight Lines of the Two Voyager Spacecraft with HST/STIS
• Transient X-ray Emission from Normal Galactic Nuclei
• Spatial Variations of the Extinction Law in the Galactic Disk from Infrared Observations
• The Herschel Virgo Cluster Survey. XIX. Physical properties of low luminosity FIR sources at $z<$ 0.5
• Detection of 3.3 Micron Aromatic Feature in the Supernova Remnant N49 with AKARI
• Metal-Enriched Outflows in the Ultra-Luminous infrared Quasar Q1321+058
• Reddening and He I* $\lambda 10830$ Absorption Lines in Three Narrow-line Seyfert 1 Galaxies
• CO isotopolog line fluxes of viscously evolving disks: cold CO conversion insufficient to explain observed low fluxes
• VLA observations of the disk around the young brown dwarf 2MASS J044427+2512
• Extinction and Distance to Anomalous X-ray Pulsars from X-ray Scattering Halos
• New Spatially Resolved Imaging of the SR 21 Transition Disk and Constraints on the Small-Grain Disk Geometry
• Planet-induced disk structures: A comparison between (sub)mm and infrared radiation
• Molecular Hydrogen Formation During Dense Interstellar Cloud Collapse
• First L band detection of hot exozodiacal dust with VLTI/MATISSE
• Unravelling the Dust Attenuation Scaling Relations and their Evolution
• Spectropolarimetric Constraints on the Nature of Interstellar Grains
• Merged H/H2 and C+/C/CO transitions in the Orion Bar
• Molecular Hydrogen in Orion as Observed by the Far Ultraviolet Spectroscopic Explorer
• Far-Ultraviolet Cooling Features of the Antlia Supernova Remnant
• A new analytical scattering phase function for interstellar dust
• Spitzer and near-infrared observations of a new bi-polar protostellar outflow in the Rosette Molecular Cloud
• Fully Sampled Maps of Ices and Silicates in Front of Cepheus A East with Spitzer
• SPAMCART: a code for smoothed particle Monte Carlo radiative transfer
• Will ALMA Reveal the True Core Mass Function of Protoclusters?
• Cosmic Reionization On Computers. Ultraviolet Continuum Slopes and Dust Opacities in High Redshift Galaxies
• The Evolution of Density Structure of Starless and Protostellar Cores
• Flux sensitivity requirements for the detection of Lyman continuum radiation drop-ins from star-forming galaxies below redshifts of 3
• JWST observations of the Horsehead photon-dominated region I. First results from multi-band near- and mid-infrared imaging
• An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS
• Dust in High-Redshift Galaxies: Reconciling UV Attenuation and IR Emission
• Implications of Grain Size Distribution and Composition for the Correlation Between Dust Extinction and Emissivity
• Pebbles in an Embedded Protostellar Disk: The Case of CB26
• Non-LTE dust nucleation in sub-saturated vapors
• Radiative transfer modelling of parsec-scale dusty warped discs
• Modeling anomalous extinction using nanodiamonds
• The Interstellar Extinction Toward the Milky Way Bulge with Planetary Nebulae, Red Clump, and RR Lyrae stars
• Anatomy of the massive star-forming region S106: The OI 63 micron line observed with GREAT/SOFIA as a versatile diagnostic tool for the evolution of massive stars
• The protoplanetary disc around HD 169142: circumstellar or circumbinary?
• The long-period Galactic Cepheid RS Puppis - II. 3D structure and mass of the nebula from VLT/FORS polarimetry
• Resolved star formation in the metal poor star-forming region Magellanic Bridge C
• The Effects of Clumping on Derived Abundances in H II Regions
• Observations of Free-Free and Anomalous Microwave Emission from LDN 1622 with the 100 m Green Bank Telescope
• Variation in the stellar initial mass function from the chromospheric activity of M dwarfs in early-type galaxies
• Constraints on observing brightness asymmetries in protoplanetary disks at solar system scale
• Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
• A Multiwavelength Study of Young Massive Star-Forming Regions. III. Mid-Infrared Emission
• Effects of dust abundance on the far-infrared colours of blue compact dwarf galaxies
• Origin and Evolution of Angular Momentum of Class II Disks
• Grain Alignment in OMC1 as Deduced from Observed Large Circular Polarization
• Constraints on interstellar dust models from extinction and spectro-polarimetry
• Chemical Kinetics Simulations of Ice Chemistry on Porous Versus Non-Porous Dust Grains
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Si and Fe depletion in Galactic star-forming regions observed by the Spitzer Space Telescope
• Dense molecular cloud cores as a source of micrometer-sized grains in galaxies
• The nature of HHL 73 from optical imaging and Integral Field Spectroscopy
• A Study of the X-Ray Dust Scattering Halo of Cyg X-1 with a Cross-Correlation Method
• Modelling of mid-infrared interferometric signature of hot exozodiacal dust emission
• On the equivalent width of the Fe K$\alpha$ line produced by a dusty absorber in active galactic nuclei
• X-ray Scattered Halo around IGR J17544-2619
• Gamma-ray Burst Afterglows: Time-Varying Extinction, Polarization, and Colors due to Rotational Disruption of Dust Grains
• Polarization reversal of scattered thermal dust emission in protoplanetary disks at (sub-)mm wavelengths
• Optical and UV surface brightness of translucent dark nebulae: Dust albedo, radiation field and fluorescence emission by H2
• Nanodust in the Interstellar Medium in Comparison to the Solar System
• How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks
• Infrared dust echoes from neutron star mergers
• The mid-infrared extinction in molecular clouds Case study of B 335
• Faint warm debris disks around nearby bright stars explored by AKARI and IRSF
• Evolution of the grain size distribution in Milky Way-like galaxies in post-processed IllustrisTNG simulations
• Are the Formation and Abundances of Metal-Poor Stars the Result of Dust Dynamics?
• Helium Ionization in the Diffuse Ionized Gas surrounding UCHII regions
• Spectral energy distributions of dust and PAHs based on the evolution of grain size distribution in galaxies
• Impact of Dust on Spectral Distortion Measurements of the Cosmic Microwave Background
• [Fe II] 1.64 um Features of Jets and Outflows from Young Stellar Objects in the Carina Nebula
• The consequence of a new ISRF model of the Milky Way on predictions for diffuse gamma-ray emission
• Spitzer IRAC Color Diagnostics for Extended Emission in Star Forming Regions
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• Dust in the Wolf-Rayet Nebula M1-67
• Spitzer Spectroscopy of the Circumprimary Disk in the Binary Brown Dwarf 2MASS J04414489+2301513
• The nature of Damped Lyman-α and MgII absorbers explored with their dust contents
• GK Car and GZ Nor: Two low-luminous, depleted RV Tauri stars
• On Carbon Nanotubes in the Interstellar Medium
• Revealing a main-sequence star that consumed a planet with JWST
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• Searching for Debris Disks around Seven Radio Pulsars
• Dust properties of the cometary globule Barnard 207 (LDN 1489)
• Evolution of dust grain size distribution and grain porosity in galaxies
• SOFIA {\it FORCAST} Photometry of 12 Extended Green Objects in the Milky Way
• Dust properties along anomalous extinction sightlines. II. Studying extinction curves with dust models
• Dust growth by accretion of molecules in supersonic interstellar turbulence
• Multi-wavelength modelling of the circumstellar environment of the massive proto-star AFGL 2591 VLA 3
• Limits on Intergalactic Dust During Reionization
• Mid-infrared imaging of Supernova 1987A
• Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
• A PDR model for the FIR mid-$J$ CO ladder with universal rotational temperature in star forming region
• Laboratory-based sticking coefficients for ices on a variety of small grains analogs
• Observational Signatures of Circumbinary Discs I: Kinematics
• Far-ultraviolet Dust Extinction and Molecular Hydrogen in the Diffuse Milky Way Interstellar Medium
• Binary astrometric microlensing with Gaia
• Probing the ambient medium of GRB 090618 with XMM-Newton observations
• Restructuring and destruction of hydrocarbon dust in the interstellar medium
• The Mid-Infrared Polarization of the Herbig Ae Star WL 16: An Interstellar Origin?
• A new Herschel view of the young star T54: not a transitional disk?
• Analytic models of dust temperature in high-redshift galaxies
• The Cold Dust Content of the Oxygen-Rich Supernova Remnant G292.0+1.8
• A Wide-Field Near-Ir H2 2.122$\mu$m line survey of the Braid Nebula Star Formation Region in Cygnus OB7
• The dust effects on galaxy scaling relations
• Relation between parameters of dust and parameters of molecular and atomic gas in extragalactic star-forming regions
• The Photolysis of Aromatic Hydrocarbons Adsorbed on the Surfaces of Cosmic Dust Grains
• The complex infrared dust continuum emission of NGC1068: ground-based N- and Q-band spectroscopy and new radiative transfer models
• Constraining the Dust Opacity Law in Three Small and Isolated Molecular Clouds
• A model grid for the reflected light from transition disks
• Understanding discs in binary YSOs: detailed modelling of VV CrA
• Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
• A low-luminosity type-1 QSO sample: IV. Molecular gas contents and conditions of star formation in three nearby Seyfert galaxies
• Modelling the spinning dust emission from LDN 1780
• The effect of grain size distribution on H${}_2$ formation rate in the interstellar medium
• On the origin of radio-loudness in active galactic nuclei using far-infrared polarimetric observations
• Rescued from oblivion: detailed analysis of archival {\it Spitzer} data of SN~1993J
• Dust Models for the Extinction of Type IIn Supernova SN 2010jl
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Combined constraints on intergalactic dust from quasar colours and the soft X-ray background
• Modeling IR Spectral Energy Distributions: A Pilot Study of Starburst Parameters and Silicate Absorption Curves for Some GOALS Galaxies
• PDRs4All. V. Modelling the dust evolution across the illuminated edge of the Orion Bar
• Investigating the ultraviolet and infrared radiation through the turbulent life of molecular clouds
• The edge-on disk Tau042021: icy grains at high altitudes and a wind containing astronomical PAHs
• Physical conditions for dust grain alignment in Class 0 protostellar cores II. The role of the radiation field in models aligning/disrupting dust grains
• A new ionisation network and radiation transport module in PLUTO
• Multiline observations of hydrogen, helium, and carbon radio-recombination lines toward Orion A: A detailed dynamical study and direct determination of physical conditions
• Ice features of low-luminosity protostars in near-infrared spectra of AKARI/IRC
• Coeval intermediate-mass star formation in N4W
• Correlation between UV resilience and wavelength of narrow DIBs
• A systematic study of ULIRGs using near-infrared absorption bands reveals a strong UV environment in their star-forming regions
• Accurate Measurement of the Lensing Magnification by BOSS CMASS Galaxies and Its Implications for Cosmology and Dark Matter
• The weak INTEGRAL bursts GRB040223 and GRB040624: an emerging population of dark afterglows
• Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift $z=0$
• $\text{Herschel}$ Photometric Observations of $\mathrm{L}\mathrm{ITTLE}$ $\mathrm{T}\mathrm{HINGS}$ Dwarf Galaxies
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Global distribution of far-ultraviolet emissions from highly ionized gas in the Milky Way
• Far-Ultraviolet Dust Albedo Measurements in the Upper Scorpius Cloud Using the SPINR Sounding Rocket Experiment
• Probing star formation and ISM properties using galaxy disk inclination III: Evolution in dust opacity and clumpiness between redshift 0.0 < z < 0.7 constrained from UV to NIR
• Ortho-to-Para Ratio Studies of Shocked H2 Gas in the Two Supernova Remnants IC 443 and HB 21
• The Acoustic Resonant Drag Instability with a Spectrum of Grain Sizes
• Tree-based solvers for adaptive mesh refinement code FLASH -- III: a novel scheme for radiation pressure on dust and gas and radiative transfer from diffuse sources
• Grain Physics and Rosseland Mean Opacities
• A deep multi-band investigation of IC2391
• Cross section alignment of polycyclic aromatic hydrocarbons by anisotropic radiation
• Dust Extinction towards the Type Ia Supernova 2012cu in NGC 4772
• Compact dusty clouds and efficient H${}_2$ formation in diffuse ISM
• Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova
• Radiative Transfer Modeling of An SN 1987A Light Echo$-$AT2019xis
• Reassessing Dust's Role in Forming the CMB
• Infrared Studies of Molecular Shocks in the Supernova Remnant HB 21: II. Thermal Admixture of Shocked H${}_2$ Gas in the South
• Extended, Dusty Star Formation Fueled by a Residual Cooling Flow in the Cluster of Galaxies Sersic 159-03
• Eddington Ratios of Dust-obscured Quasars at $z\lesssim 1$: Evidence Supporting Dust-obscured Quasars as Young Quasars
• Comparing Galaxy Clustering in Horizon-AGN Simulated Lightcone Mocks and VIDEO Observations
• Supernova dust destruction in the magnetized turbulent ISM
• Far Ultraviolet Diffuse Emission from the Large Magellanic Cloud
• Spatially resolved [CII]-gas conversion factor in early galaxies
• Cosmic evolution of grain size distribution in galaxies using the ${\nu }^2$GC semi-analytic model
• Photometric Redshifts of Submillimeter Galaxies
• Spitzer and Herschel studies of dust in supernova remnants in the Small Magellanic Cloud
• Using deuterated H3+ and other molecular species to understand the formation of stars and planets
• Cosmological X-ray Scattering from Intergalactic Dust
• Polarization as a probe of thick dust disk in edge-on galaxies: application to NGC 891
• Constraining Spatial Densities of Early Ice Formation in Small Dense Molecular Cores from Extinction Maps
• Orientation effect on the ligh curve shape of periodic methanol maser sources
• Effects of dust grain size distribution on the abundances of CO and H${}_2$ in galaxy evolution
• The HP2 Survey - IV. The Pipe nebula: Effective dust temperatures in dense cores
• Modelling H${}_2$ and its effects on star formation using a joint implementation of GADGET-3 and KROME
• Modelling thermochemical processes in protoplanetary disks I: numerical methods
• Interstellar absorption and dust scattering
• Synergies between interstellar dust and heliospheric science with an Interstellar Probe
• Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
• Importance of far-infrared mapping in a spiral galaxy: AKARI observation of M81
• WISE Discovery of Mid-infrared Variability in Massive Young Stellar Objects
• A deep optical/near-infrared catalog of Serpens
• Ultraviolet extinction properties of the 30 Dor Nebula and interpreting observations of starburst clusters
• Radial profiles of lensed $z\sim 1$ galaxies on sub-kiloparsec scales
• Modelling galaxy spectra in presence of interstellar dust-III. From nearby galaxies to the distant Universe
• A Mystery in Chamaeleon: Serendipitous Discovery of a Galactic Symbiotic Nova
• Effects of rotational disruption on the evolution of grain size distribution in galaxies
• Non-explosive pre-supernova feedback in the COLIBRE model of galaxy formation
• Modeling the Vertical Structure of Nuclear Starburst Discs: A Possible Source of AGN Obscuration at $z\sim 1$
• Observational signatures of the dust size evolution in isolated galaxy simulations
• Dust Heating by Low-mass Stars in Massive Galaxies at z<1
• Radiation Effects from ISM and Cosmic Ray Particle Impacts on Relativistic Spacecraft
• Very Large Telescope observations of Gomez's Hamburger: Insights into a young protoplanet candidate
• Extinction Laws toward Stellar Sources within a Dusty Circimstellar Medium and Implications for Type Ia Supernovae
• Primordial dust rings, hidden dust mass, and the first generation of planetesimals in gravitationally unstable protoplanetary disks
• Evidence for a Dusty Dark Dwarf Galaxy in the Quadruple Lens MG0414+0534
• Testing the Potential for Radio Variability in Disks around T Tauri Stars with Observations and Chemical Modeling
• Shattering as a source of small grains in the circum-galactic medium
• Variability of Disk Emission in Pre-Main Sequence and related Stars. V. Occultation Events from the innermost disk region of the Herbig Ae Star HD 163296
• The incidence of mid-infrared excesses in G and K giants
• Infrared Spectroscopic Survey of the Quiescent Medium of Nearby Clouds: II. Ice Formation and Grain Growth in Perseus and Serpens
• Characterization of mid-infrared polarization due to scattering in protoplanetary disks
• CARMA Observations of Galactic Cold Cores: Searching for Spinning Dust Emission
• Identification of emission-line stars in transition phase from pre-main sequence to main sequence
• The advantages of using a Lucky Imaging camera for observations of microlensing events
• Polarimetry of the potential binary supermassive black hole system in J1430+2303
• Influence of the nano-grain depletion in photon-dominated regions: Application to the gas physics and chemistry in the Horsehead
• UV-controlled physical and chemical structure of protoplanetary disks
• A mid-infrared study of HII regions in the Magellanic Clouds: N88A and N160A
• Massive black holes in high-redshift Lyman Break Galaxies
• H${}_2$O Maser Pumping: The Effect of Quasi-Resonance Energy Transfer in Collisions between H${}_2$ and H${}_2$O Molecules
• HOPS 361-C's Jet Decelerating and Precessing Through NGC 2071 IR
• The Effect of Warm Dark Matter on Early Star Formation Histories of Massive Galaxies: Predictions from the CROC Simulations
• Observations of Far-Ultraviolet Diffuse Emission from the Small Magellanic Cloud
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Dust Attenuation Curve for Local Subgalactic Star-forming Regions
• The role of external FUV irradiation in the survival of astrophysical ices in Elias 29
• Evidence for anomalous dust-correlated emission at 8 GHz
• IRS Characterization of a Debris Disk around an M-type star in NGC2547
• On the Properties of the Galactic Dust Layer within 700 pc of the Sun
• The grey extinction of the ionizing cluster in NGC 3603 from ultraviolet to optical wavelengths
• Constraints on the dust extinction law of the Galaxy with Swift/UVOT, Gaia and 2MASS
• Extinction towards the cluster R136 in the Large Magellanic Cloud: An extinction law from the near-infrared to the ultraviolet
• Variations of the ISM Compactness Across the Main Sequence of Star-Forming Galaxies: Observations and Simulations
• Photon Feedback: Screening and the Eddington Limit
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• Effect of Dust on Lyman-alpha Photon Transfer in Optically Thick Halo
• A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
• A census of young stellar objects in two line-of-sight star forming regions toward IRAS 22147+5948 in the outer Galaxy
• Predicting HCN, HCO + , multi-transition CO, and dust emission of star-forming galaxies: Constraining the properties of resolved gas and dust disks of local spiral galaxies
• An independent determination of the distance to supernova SN 1987A by means of the light echo AT 2019xis
• JWST captures a sudden stellar outburst and inner disk wall destruction
• 94 Ceti: a triple star with a planet and dust disc
• The Composite Spectral Energy Distribution of Quasars is Surprisingly Universal Since Cosmic Noon
• The Formation and Evolution of Massive Stellar Clusters in IC 4662
• Mid-IR FORCAST/SOFIA Observations of M82
• Dust in the Local Group
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• An analysis of the FIR/RADIO Continuum Correlation in the Small Magellanic Cloud
• On the Absorption Properties of Metallic Needles
• The rotational disruption of porous dust aggregates from ab-initio kinematic calculations
• The Impact of Light Polarization Effects on Weak Lensing Systematics
• Decoding NGC 628 with radiative transfer methods
• Signatures of reionization feedback in the near-infrared background
• Simulation of a strategy for the pixel lensing of M87 using the Hubble Space Telescope
• Modelling Grain Rotational Disruption by Radiative Torques and Extinction of Active Galactic Nuclei
• Gas physical conditions and kinematics of the giant outflow Ou4
• Weak lensing magnification of Type Ia Supernovae from the Pantheon sample
• [Fe II] 1.64 um Imaging Observations of the Outflow Features around Ultracompact H II Regions in the 1st Galactic Quadrant
• A Comparison of Approaches in Fitting Continuum SEDs
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Interstellar Dust models towards some IUE stars
• Interstellar Dust and Gas in the Heliosphere
• Linking ice and gas in the Coronet cluster in Corona Australis
• The Cosmic-Ray Induced Sputtering Process On Icy Grains
• LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit
• Deriving the intrinsic properties of M51 with radiative transfer models
• Near-infrared scattering as a dust diagnostic
• Brilliant Pebbles: A Method for Detection of Very Large Interstellar Grains
• Monte Carlo post-processing for radiation hydro simulations of accreting planets in protoplanetary disks
• On the optical properties of Resonant Drag Instabilities: Variability of Asymptotic Giant Branch and R Coronae Borealis stars
• The Largest Fullerene
• Molecular Jets from an Evolved Protostar: Insights from JWST-ALMA Synergy
• Modelling LAEs in the Epoch of Reionization with OBELISK
• Massive Protocluster of a Periodic Maser Source G188.95+0.89
• Gaseous nebulae and massive stars in the giant HI ring in Leo
• A tiny Galactic dust cloud projected onto NGC 3269?
• The Galactic Center in Color: Measuring Extinction with High-Proper-Motion Stars
• The first radio spectrum of a rapidly rotating A-type star
• Chemical properties of two dense cores in a Planck Galactic Cold Clump G168.72-15.48
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Synthetic extinction maps around intermediate-mass black holes in Galactic globular clusters
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
• Optical properties of elongated conducting grains
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Optical Properties of Interstellar Dust around the Orion A Molecular Cloud
• Wavelength-Dependent Extinction and Grain Sizes in Dippers
• Resonant Drag Instabilities for Polydisperse Dust, I. The Acoustic Resonant Drag Instability
• The 2175 Å~ Bump Features in FeLoBAL Quasars: One Indicator of MW-like Dust in the Nuclear Region of Quasar
• A Pop III generated dust screen at z~16
• Radiation-driven dusty outflows from early galaxies
• Unveiling dust, molecular gas, and high star formation efficiency in extremely UV bright star-forming galaxies at $z\sim 2.1-3.6$
• Dust Mass Associated with the Supernova Remnant IC 443 when Emission Meets Extinction
• The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
• Disk dissipation, giant planet formation and star-formation-rate fluctuations in the past three-million-year history of Gould's Belt
• Evolving grain-size distributions embedded in gas flows
• Full disc [CII] mapping of nearby star-forming galaxies: SOFIA FIFI/LS observations of NGC 3627, NGC 4321, and NGC 6946
• Uncovering the truth about M101, NGC 3938, and their significant others through radiative transfer
• On the Late-Time Spectral Softening Found in X-ray Afterglows of Gamma-Ray Bursts
• The accretion luminosity of Class I protostars
• On the scaling relations of bulges and early-type galaxies
• The dust properties of z ~ 3 MIPS-LBGs from photo-chemical models
• Synthetic observations of protostellar multiple systems
• Hot exozodiacal dust around Fomalhaut: The MATISSE perspective
• The Interaction of Supernova Remnant G357.7+0.3 with the Interstellar Medium
• The Disappearing Envelope around the Transitional Class I Object L43
• SRG/eROSITA 3D mapping of the ISM using X-ray absorption spectroscopy
• Photometric Identification of Objects from Galaxy Evolution Explorer Survey and Sloan Digital Sky Survey
• Impact of hot exozodiacal dust on the polarimetric analysis of close-in exoplanets
• Global Spectral Energy Distributions of the Large Magellanic Cloud with Interstellar Dust
• Dust growth in molecular cloud envelopes: a numerical approach
• Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K-primaries -- II: Carbon, oxygen, and odd-Z iron-peak abundances of the primary stars
• Dust Evolution in Simulated Multiphase Galactic Outflows
• Physically motivated modeling of LyC escape fraction during reionization
• Synthetic ngVLA line observations of a massive star-forming cloud
• Limits on Polarized Dust Spectral Index Variations for CMB Foreground Analysis
• Dense cores in the Seahorse infrared dark cloud: physical properties from modified blackbody fits to the far-infrared-submillimetre spectral energy distributions
• On planet formation around supermassive black holes and the grain disruption barriers by radiative torques
• Optical properties and dust temperatures in clumpy diffuse medium
• The potential of combining MATISSE and ALMA observations: Constraining the structure of the innermost region in protoplanetary discs
• Passage of a Gamma-Ray Burst Through a Molecular Cloud: Cloud Ionization Structure
• The Correlation Between Dust and Gas Contents in Molecular Clouds
• Nebular Dust Attenuation with the Balmer and Paschen Lines based on the MaNGA Survey
• From small dust to micron-sized aggregates: the influence of structure and composition on the dust optical properties
• Bright stars observed by FIMS/SPEAR
• Silicon and iron dust in gamma-ray burst host galaxy absorbers
• Considering light-matter interactions in the Friedmann equations
• The origin and evolution of the [CII] deficit in HII regions and star-forming molecular clouds
• Extra-Solar Kuiper Belt Dust Disks
• GATOS XI : Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI
• Dust emission and extinction in the Orion OMC-3 cloud
• CHESS: an Innovative Concept for High-Resolution, Far-UV Spectroscopy
• A Mysterious Ring in Dark Space?
• AstroSat/UVIT Study of the Diffuse Ultraviolet Radiation in the Dwarf Galaxy Holmberg II
• The dust-star interplay in late-type galaxies at z < 0.5: forecasts for the JWST
• Limitations of the modified blackbody fit method for determining molecular cloud properties
• Herschel/PACS photometry of transiting-planet host stars with candidate warm debris disks
• New X-ray Selected Pre-Main Sequence Members of the Serpens Molecular Cloud
• The Anomalous 21-cm Absorption at High Redshifts
• A Massive Gas Outflow Outside the Line-of-Sight: Imaging Polarimetry of the Blue Excess Hot Dust Obscured Galaxy W0204-0506
• Mid-infrared extinction curve for protostellar envelopes from JWST-detected embedded jet emission: the case of TMC1A
• The extremely truncated circumstellar disc of V410 X-ray 1: a precursor to TRAPPIST-1?
• Deuterium fractionation of the starless core L 1498
• Geometrical Distance Determination using Type I X-ray Bursts
• Spinning Nanoparticles Impacted by C-shock: Implications for Radio-millimeter Emission from Star-forming Regions
• Mid-infrared absorption spectra and mass absorption coefficients for 23 chondrites: dependence on composition and grain size
• Impact of ice growth on the physical and chemical properties of dense cloud cores
• Modelling the SEDs of spiral galaxies
• Reconstructing galaxy star formation histories from COSMOS2020 photometry using simulation-based inference
• The JCMT Transient Survey: Four Year Summary of Monitoring the Submillimeter Variability of Protostars
• Probing the infrared counterparts of diffuse far-ultraviolet sources in the Galaxy
• RR Lyrae stars with variable mean magnitudes
• The potential of VLTI observations for the study of circumstellar disk variability
• JWST Observations of Starbursts: Dust Processing in the M82 Superwind
• Towards an observationally motivated AGN dusty torus model -- II. The roles of density distribution and chemical composition of the dust
• A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
• Equivalence of light transport and depolarization
• First Light And Reionisation Epoch Simulations (FLARES) III: The properties of massive dusty galaxies at cosmic dawn
• Clustering Diffused-Particle Method for Scattering from Large Ensembles of Electromagnetically Polarizable Particles
• A physically-motivated template set for high-z galaxy SED fitting
• Far-infrared to centimeter emission of very nearby galaxies with archival data
• Nuclear astrophysics
• Shape Analysis of HII Regions -- II. Synthetic Observations
• MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
• Time-Varying Extinction, Polarization, and Colors of Type Ia Supernovae due to Rotational Disruption of Dust Grains
• Organic Acid Chemistry in ISM: Detection of Formic Acid and its Prebiotic Chemistry in Hot Core G358.93$-$0.03 MM1
• Quantitative Morphology of Galactic Cirrus in Deep Optical Imaging
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
• When did the initial mass function become bottom-heavy?
• Implications of scattering for CMB foreground emission modelling
• Extreme Starlight Polarization Efficiency Toward $\zeta$ Ophiuchi: A Case for Line-of-Sight Foreground Subtraction
• Observation of an Accreting Planetary-Mass Companion with Signs of Disk-Disk Interaction in Orion
• How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations
• Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
• Interstellar Grains: Effect of Inclusions on Extinction
• LHAASO Galactic Plane $\gamma$-rays Strongly Constrain Heavy Dark Matter
• SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths
• PDRs4All XVII: Formation and excitation of HD in photodissociation regions. Application to the Orion Bar
• Hydrogen recombination near-infrared line mapping of Centaurus A with IRSF/SIRIUS
• Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$
• Infrared observations of the flaring maser source G358.93-0.03 -- SOFIA confirms an accretion burst from a massive young stellar object
• Modeling Two First Hydrostatic Core Candidates Barnard 1b-N and 1b-S
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Analysis of Galactic cirrus filaments in HSC-SSP high-resolution deep images using artificial neural networks
• LISA Galactic Binaries in the Roman Galactic Bulge Time-Domain Survey
• GRB 180325A: dust grain-size distribution and interstellar iron nanoparticles contribution
• Impact of an inhomogeneous density distribution on selected observational characteristics of circumstellar disks
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• Origin and evolution of the Galactic inventories of interstellar dust and its composition
• Spitzer IRAC Colors of Nebulae Associated with Star-Forming Regions
• Diverse reddening distributions in sight lines to type Ia supernovae
• A study of frequency and size distribution dependence of extinction for astronomical silicate and graphite grains
• The PRIMA promise of deciphering interstellar dust evolution with observations of the nearby Universe
• Interstellar dust as a dynamic environment
• An Improved Pair Method to Probe the Dust Extinction Law
• First studies of the diffuse X-ray emission in the Large Magellanic Cloud with eROSITA
• The optical constants and grain sizes of interstellar dust measured directly using the dust scattered x-ray halo of GRB 221009A
• Massive Star and Star Cluster Formation
• Probing Interstellar Dust With Space-Based Coronagraphs
• What is the amount of baryonic dark matter in galaxies?
• A Semi-Empirical Model of the Infrared Emission from Galaxies
• The MATISSE view of the inner region of the RY Tau protoplanetary disk
• Feasibility of interferometric observations and characterization of planet-induced structures at sub au to au scales in protoplanetary disks
• "Ashfall" Induced by Molecular Outflow in Protostar Evolution. II. Analytical Study on the Maximum Size of Dust Grains Lifted by Outflows
• H2 MAGIE: H2 as a Major Agent to Galaxy Interaction and Evolution
• The effect of carbon grain destruction on the chemical structure of protoplanetary disks
• Linking simulations and observations of star-forming regions I. Masses and temperatures of ALMAGAL-like cores
• An Agnostic Approach to Building Empirical Type Ia Supernova Light Curves: Evidence for Intrinsic Chromatic Flux Variation Using Nearby Supernova Factory Data
• PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
• The Substructures in Disks undergoing Vertical Shear Instability: II. Observational Predictions for the Dust Continuum
• ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229
• Tricolor Technique for Visualization of Spatial Variations of Polydisperse Dust in Gas-Dust Flows
• A new model of composite interstellar dust grains
• Optical constants of Ih, Ic, and amorphous H${}_2$O ices in the THz and IR ranges
• Dense Star-forming Gas and Dust in the Magellanic Clouds
• TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane
• A Detailed Analysis of Intermediate-scale Structure in Optical Extinction Curves: Expanded Census and Two-family Classification
• Analytic formulas for frequency and size dependence of absorption and scattering efficiencies of astronomical polycyclic aromatic hydrocarbons
• Constraining the Metallicities of Damped Ly$\alpha$ Systems Using Extinction Curves
• Effect of dust in circumgalactic haloes on the cosmic shear power spectrum
• Dust and inclination corrected star-formation and interstellar medium scaling relations in nearby galaxies
• Can CCM law properly represent all extinction curves?