Infrared Emission from Interstellar Dust. II. The Diffuse Interstellar Medium

Abstract

We present a quantitative model for the infrared emission from dust in the diffuse interstellar medium. The model consists of a mixture of amorphous silicate grains and carbonaceous grains, each with a wide size distribution ranging from molecules containing tens of atoms to large grains > 1 um in diameter. We assume that the carbonaceous grains have polycyclic aromatic hydrocarbon (PAH)-like properties at very small sizes, and graphitic properties for radii a > 50 A. On the basis of recent laboratory studies and guided by astronomical observations, we propose "astronomical" absorption cross sections for use in modeling neutral and ionized PAHs from the far ultraviolet to the far infrared. We also propose modifications to the far-infrared emissivity of "astronomical silicate". We calculate energy distribution functions for small grains undergoing "temperature spikes" due to stochastic absorption of starlight photons, using realistic heat capacities and optical properties. Using a grain size distribution consistent with the observed interstellar extinction, we are able to reproduce the near-IR to submillimeter emission spectrum of the diffuse interstellar medium, including the PAH emission features at 3.3, 6.2, 7.7, 8.6, and 11.3um. The model is compared with the observed emission at high Galactic latitudes as well as in the Galactic plane, as measured by COBE and IRTS. We calculate infrared emission spectra for our dust model heated by a range of starlight intensities, and we provide tabulated dust opacities (extended tables available at http://www.astro.princeton.edu/~draine/dust/dustmix.html)

Final version published in ApJ, 554, 778 but with factor 1.086 error in Table 6 and Fig. 16 corrected. Main change from astro-ph version 1 is correction of typographical errors in Table 1, and correction of typo in eq. (A2). 51 pages, 16 figures, Latex

References in corpus (5)

• Infrared Emission from Interstellar Dust. I. Stochastic Heating of Small Grains
• The CH out-of-plane bending modes of PAH molecules in astrophysical environments
• On Ultrasmall Silicate Grains in the Diffuse Interstellar Medium
• Forces on Dust Grains Exposed to Anisotropic Interstellar Radiation Fields
• Unidentified Infrared Emission Bands in the Diffuse Interstellar Medium

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• Simulating the diversity of shapes of the Lyman-$\alpha$ line
• On the Morphology and Chemical Composition of the HR 4796A Debris Disk
• The Molecular Interstellar Medium of the Local Group Dwarf NGC6822
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• Search for corannulene (C20H10) in the Red Rectangle
• The Circumstellar Environment of R Coronae Borealis: White Dwarf Merger or Final Helium Shell Flash?
• The Mipsgal View of Supernova Remnants in the Galactic Plane
• Probing the Nuclear and Circumnuclear Activity of NGC1365 in the Infrared
• Dust Emission from the Perseus Molecular Cloud
• [CII] emission from L1630 in the Orion B molecular cloud
• Gas lines from the 5-Myr old optically thin disk around HD141569A. Herschel observations and modeling
• T-carbon: experiments, properties, derivatives and potential applications
• Modelling galaxy spectra in presence of interstellar dust. I. The model of ISM and the library of dusty SSPs
• Spitzer and JCMT Observations of the Active Galactic Nucleus in the Sombrero Galaxy (NGC 4594)
• Molecular gas properties of a lensed star-forming galaxy at z~3.6: a case study
• Simulating radiative feedback and star cluster formation in GMCs: I. Dependence on gravitational boundedness
• Star formation around the HII region Sh2-235
• A multi-wavelength investigation of RCW175: an HII region harboring spinning dust emission
• The thermal emission of Centaurs and Trans-Neptunian objects at millimeter wavelengths from ALMA observations
• Probing the Excitation of Extreme Starbursts: High Resolution Mid-IR Spectroscopy of Blue Compact Dwarfs
• Starburst--driven galactic outflows
• Constraint on the Polarization of Electric Dipole Emission from Spinning Dust
• The Spectrum of Integrated Millimeter Flux of the Magellanic Clouds and 30-Doradus from TopHat and DIRBE Data
• NOEMA redshift measurements of bright Herschel galaxies
• What produces the far-infrared/submm emission in the most luminous QSOs?
• A Dust spectral energy distribution model with hierarchical Bayesian inference. I. Formalism & benchmarking
• Spitzer Analysis of HII Region Complexes in the Magellanic Clouds: Determining a Suitable Monochromatic Obscured Star Formation Indicator
• Simulations of protostellar collapse using multigroup radiation hydrodynamics. I. The first collapse
• Large-scale Star Formation Triggering in the Low-mass Arp 82 System: A Nearby Example of Galaxy Downsizing Based on UV/Optical/Mid-IR Imaging
• Probing the Protostellar Envelope around L1157: the Dust and Gas Connection
• PHANGS-JWST First Results: Tracing the Diffuse ISM with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies
• Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Infrared Spectral Energy Distribution Model for Extremely Young Galaxies
• Variation of the extinction law in the Trifid nebula
• Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations
• Full SED fitting with the KOSMA-τ PDR code - I. Dust modelling
• Mid-Infrared Spectroscopy of Infrared Luminous Galaxies with Sub-Arcsecond Resolution
• Evolution of the extinction curves in galaxies
• Interstellar extinction and interstellar polarization: old and new models
• Sensitivity of PDR Calculations to Microphysical Details
• The Extreme Star Formation Activity of Arp299 Revealed by Spitzer IRS Spectral Mapping
• Effects of grain growth mechanisms on the extinction curve and the metal depletion in the interstellar medium
• The Spatial Distribution of Dust and Stellar Emission of the Magellanic Clouds
• The Interstellar Oxygen Crisis, or Where Have All the Oxygen Atoms Gone?
• Probing the Role of Carbon in the Interstellar Ultraviolet Extinction
• Spatially Resolved 3 micron Spectroscopy of Elias 1: Origin of Diamonds in Protoplanetary Disks
• High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030
• Extinction curve template for intrinsically reddened quasars
• Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck
• Properties of Starless and Prestellar Cores in Taurus Revealed by Herschel SPIRE/PACS Imaging
• The Carriers of the "Unidentified" Infrared Emission Features: Clues from Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups
• A Tale of Two Mysteries in Interstellar Astrophysics: The 2175 Angstrom Extinction Bump and Diffuse Interstellar Bands
• The evolution of actively star forming galaxies in the mid infrared
• Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties
• Constraining dust formation in high-redshift young galaxies
• The Herschel Virgo cluster survey: V. Star-forming dwarf galaxies - dust in metal-poor environments
• Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z~1
• Far-infrared Observations of the Very Low-Luminosity Embedded Source L1521F-IRS in the Taurus Star-Forming Region
• Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
• Extinction Correction for Type Ia Supernova Rates. I. The Model
• On The Gas Temperature of Molecular Cloud Cores
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• The Spatially Resolved Dust-to-Metals Ratio in M101
• Spinning dust emission from ultrasmall silicates: emissivity and polarization spectrum
• Gas and Star Formation in the Circinus Galaxy
• Mitigating Complex Dust Foregrounds in Future CMB Polarization Experiments
• Silicate Composition of the Interstellar Medium
• Observing Extended Sources with the \Herschel SPIRE Fourier Transform Spectrometer
• On the Flux of Extra-Solar Dust in Earth's Atmosphere
• The Mystery of Unidentified Infrared Emission Bands
• Self-consistent modelling of aromatic dust species and extinction curves in galaxy evolution
• Silicate Emission in the Spitzer IRS spectrum of FSC 10214+4724
• Candidate Water Vapor Lines to Locate the H${}_2$O Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star
• Spitzer characterisation of dust in an anomalous emission region: the Perseus cloud
• Supernovae and AGN driven galactic outflows
• The roles of star formation and AGN activity of IRS sources in the HerMES fields
• Warm Dust and Spatially Variable PAH Emission in the Dwarf Starburst Galaxy NGC 1705
• The X-Ray Scattering Halo Around Nova Cygni 1992: Testing a Model for Interstellar Dust
• On the Measurement of Elemental Abundance Ratios in Inner Galaxy H II Regions
• A chemical model for the interstellar medium in galaxies
• Shocks in dense clouds. IV. Effects of grain-grain processing on molecular line emission
• Dust formation, evolution, and obscuration effects in the very high-redshift universe
• Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk
• The Infrared Continuum Radiation of NGC1808 : A PAH and Polarisation Study
• Variations in 24 micron morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: New insights into the Hubble sequence
• Enhanced production of HD and D_2 molecules on small dust grains in diffuse clouds
• Observations of Cold Dust in Nearby Elliptical Galaxies
• Unidentified Infrared Bands in the Interstellar Medium across the Galaxy
• Towards Detecting The 2175-Å Dust Feature Associated With Strong High Redshift Mg ßII Absorption Lines
• VLT Spectropolarimetry of the optical transient in NGC300. Evidence for asymmetry in the circumstellar dust
• The gas-to-dust mass ratio of Centaurus A as seen by Herschel
• Dissecting the origin of the submillimeter emission in nearby galaxies with Herschel and LABOCA
• X-ray radiative transfer in full 3D with SKIRT
• Dual-Wavelength ALMA Observations of Dust Rings in Protoplanetary Disks
• Silicate Dust in Active Galactic Nuclei
• Variations between Dust and Gas in the Diffuse Interstellar Medium
• X-Ray Scattering by Nonspherical Grains. I. Oblate Spheroids
• Multi-phase outflows in post starburst E+A galaxies -- I. General sample properties and the prevalence of obscured starbursts
• The fate of the Antennae galaxies
• The Galactic Census of High- and Medium-mass Protostars. II. Luminosities and Evolutionary States of a Complete Sample of Dense Gas Clumps
• Star-forming accretion flows and the low luminosity nuclei of giant elliptical galaxies
• Evaluating and Improving Semi-analytic modeling of Dust in Galaxies based on Radiative Transfer Calculations II: Dust Emission in the Infrared
• Dust Extinction of Gamma-ray Burst Host Galaxies: Identification of Two Classes?
• The physical and chemical structure of Sagittarius B2 -- V. Non-thermal emission in the envelope of Sgr B2
• Mid-Infrared Spectroscopic Evidence for AGN Heating Warm Molecular Gas
• The AKARI 2.5-5 Micron Spectra of Luminous Infrared Galaxies in the Local Universe
• X-ray radiative transfer in protoplanetary disks - The role of dust and X-ray background fields
• Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
• Lyα emission from galaxies in the Epoch of Reionization
• Time-Dependent, Multifluid, Magnetohydrodynamic Shock Waves with Grain Dynamics I. Formulation and Numerical Tests
• The nuclear and extended infrared emission of the Seyfert galaxy NGC 2992 and the interacting system Arp 245
• Multigroup radiation hydrodynamics with flux-limited diffusion and adaptive mesh refinement
• Examining the class B-to-A shift of the 7.7 $\mu$m PAH band with the NASA Ames PAH IR Spectroscopic Database
• Evaporation of Low-Mass Planet Atmospheres: Multidimensional Hydrodynamics with Consistent Thermochemistry
• Mapping the interstellar medium in galaxies with Herschel/SPIRE
• First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
• Can Fluffy Dust Alleviate the "Subsolar" Interstellar Abundance Problem?
• On the stability of non-isothermal Bonnor-Ebert spheres
• The thermal dust emission in the N158-N159-N160 (LMC) star forming complex mapped by Spitzer, Herschel and LABOCA
• Spatially Resolved Spitzer Spectroscopy of the Starburst Nucleus in NGC 5253
• Spatial Distribution of Dust Grains within H II Regions
• Dust enshrouded star-forming activity in Arp 299
• Modeling the Infrared Interstellar Extinction
• Star-formation histories of local luminous infrared galaxies
• PAH Spectroscopy from 1-5 $\mu$m
• High-resolution mapping of interstellar clouds with near-infrared scattered light
• Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains
• The Origin of the 4.5 micron Excess from Dwarf Galaxies
• The Pseudo-zodi Problem for Edge-on Planetary Systems
• Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies
• Mid-Infrared Spectropolarimetric Constraints on the Core-Mantle Interstellar Dust Model
• Spiral Structure and Differential Dust Size Distribution in the LkHa 330 Disk
• Close-up view of a luminous star-forming galaxy at z=2.95
• Effects of dust scattering albedo and 2175 A bump on ultraviolet colours of normal disc galaxies
• Probing the Interstellar Dust towards the Galactic Centre: Dust Scattering Halo around AX J1745.6-2901
• GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
• The cosmic carbon footprint of massive stars stripped in binary systems
• Physical Dust Models for the Extinction toward Supernova 2014J in M82
• Measurements of Diffuse Sky Emission Components in High Galactic Latitudes at 3.5 and 4.9 um Using DIRBE and WISE Data
• Tracing the ISM magnetic field morphology: The potential of multi-wavelength polarization measurements
• Low-Resolution Spectrum of the Diffuse Galactic Light and 3.3 um PAH emission with AKARI InfraRed Camera
• A submillimeter exponential disk in M~51: evidence for an extended cold dust disk
• The Star Formation History of the Virgo early-type galaxy NGC4435: the Spitzer Mid Infrared view
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• VLT/X-shooter GRBs: Individual extinction curves of star-forming regions
• L1495 Revisited: A PPMAP View of a Star-Forming Filament
• Herschel and SCUBA-2 observations of dust emission in a sample of Planck cold clumps
• Predictions of polarized dust emission from interstellar clouds: spatial variations in the efficiency of radiative torque alignment
• Evolution of dust and molecular hydrogen in the Magellanic System
• Simulations of polarized dust emission
• Linking Characteristics of the Polycyclic Aromatic Hydrocarbon Population with Galaxy Properties: A Quantitative Approach Using the NASA Ames PAH IR Spectroscopic Database
• Shiva: the dust destruction model
• Quantifying the (X/peanut)-shaped Structure of the Milky Way - New Constraints on the Bar Geometry
• Some Stars are Totally Metal: A New Mechanism Driving Dust Across Star-Forming Clouds, and Consequences for Planets, Stars, and Galaxies
• Near-Infrared Integral Field Spectroscopy of Star-Forming Galaxies
• Molecular Hydrogen in the Ionized Region of Planetary Nebulae
• Multiband Polarimetric Imaging of HR 4796A with the Gemini Planet Imager
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Mapping and Mass Measurement of the Cold Dust in NGC 205 with Spitzer
• A relation of the PAH 3.3 um feature with star-forming activity for galaxies with a wide range of infrared luminosity
• Spitzer Observations of Cold Dust Galaxies
• Through the magnifying glass: ALMA acute viewing of the intricate nebular architecture of OH231.8+4.2
• Extra-Nuclear Starbursts: Young Luminous Hinge Clumps in Interacting Galaxies
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z~2
• Far-Infrared Properties of Blue Compact Dwarf Galaxies Observed with AKARI/Far-Infrared Surveyor (FIS)
• A Cometary Bow Shock and Mid-Infrared Emission Variations Revealed in Spitzer Observations of HD 34078 and IC 405
• Diffuse Interstellar Bands and the Ultraviolet Extinction Curves: The Missing Link Revisited
• X-ray versus Optical Observations of Active Galactic Nuclei: Evidence for Large Grains?
• GALEX UV properties of the polar ring galaxy MCG-05-07-001 and the shell galaxies NGC 1210 and NGC 5329
• On the origin of M81 group extended dust emission
• Stellar Populations and the Star Formation Histories of LSB Galaxies: IV Spitzer Surface Photometry of LSB Galaxies
• The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• A Corona Australis cloud filament seen in NIR scattered light I. Comparison with extinction of background stars
• The 3.3 micron PAH Emission as a Star Formation Rate Indicator
• Lanthanides or dust in kilonovae: lessons learned from GW170817
• Extended Emission by Dust in the Dwarf Galaxy UGC 10445
• The Bright Extragalactic ALMA Redshift Survey (BEARS) II: Millimetre photometry of gravitational lens candidates
• Constraining the ISM properties of the Cloverleaf quasar host galaxy with Herschel spectroscopy
• Structure of the interstellar medium around Cas A
• Identification of Main Sequence Stars with Mid-Infrared Excesses Using GLIMPSE: Beta-Pictoris Analogs?
• Extremely massive young clusters in NGC1365
• The Mid-Infrared [SIV]/[NeII] versus [NeIII]/[NeII] Correlation
• Dust emissivity and absorption cross section in DustPedia late-type galaxies
• Probing Cosmic Dust of the Early Universe through High-Redshift Gamma-Ray Bursts
• The Dust in M31
• Modelling galaxy spectra in presence of interstellar dust. II. From the UV to the far infrared
• The Herschel Virgo Cluster Survey. XVIII. Star-forming dwarf galaxies in a cluster environment
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3
• Infrared Emission from Intracluster Dust Grains and Constraints on Dust Properties
• The UV 2175Å Attenuation Bump and its Correlation with PAH Emission at z~2
• Dust-driven wind from disk galaxies
• Herschel observations of Cen A: stellar heating of two extragalactic dust clouds
• Uncovering Red and Dusty Ultraluminous X-ray Sources with Spitzer
• Millimeter and Submillimeter Excess Emission in M33 revealed by Planck and LABOCA
• Interstellar dust along the line of sight of GX 3+1
• An Observational Study for Grain Dynamics in the AS 209 Disk with Submillimeter Polarization
• Fundamental differences in the properties of red and blue quasars: measuring the reddening and accretion properties with X-shooter
• An Empirical Decomposition of Near-IR Emission into Galactic and Extragalactic Components
• Shattering by turbulence as a production source of very small grains
• Cosmic Needles versus Cosmic Microwave Background Radiation
• LABOCA observations of giant molecular clouds in the south west region of the Small Magellanic Cloud
• Dust Destruction by Charging: A Possible Origin of Grey Extinction Curves of Active Galactic Nuclei
• Light Echoes of Transients and Variables in the Local Universe
• Galactic Center Extinction: Evidence for Metallic Needles in the General Interstellar Medium
• An embedded active nucleus in the OH megamaser galaxy IRAS16399-0937
• Composite Interstellar Grains
• Radiative transfer of ionizing radiation through gas and dust: stellar source case
• Absorption by Spinning Dust: a Contaminant for High-Redshift 21 cm Observations
• The Modelling of InfraRed Dark Clouds
• BLAST05: Power Spectra of Bright Galactic Cirrus at Submillimeter Wavelengths
• High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
• Interstellar Silicon Depletion and the Ultraviolet Extinction
• Extinction in the 11.2 micron PAH band and the low L_11.2/L_IR in ULIRGs
• Photoelectric Heating and [CII] Cooling of High Galactic Latitude Translucent Clouds
• On Buckyonions as an Interstellar Grain Component
• On the Aliphatic versus Aromatic Content of the Carriers of the "Unidentified" Infrared Emission Features
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• [O I] 63 micron Emission from High and Low Luminosity AGN Galaxies
• Panspermia in a Milky Way-like Galaxy
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• Far-Infrared detection of neutral atomic oxygen toward the Horsehead Nebula
• Isentropic thermal instability in atomic surface layers of photodissociation regions
• Determination of the far-infrared dust opacity in a prestellar core
• Submillimeter imaging of the Galactic Center starburst Sgr B2. Warm molecular, atomic, and ionized gas far from massive star-forming cores
• Using Spitzer Colors as Diagnostics of Star Formation Regions: The Interacting Galaxy Arp 107
• Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2
• The highly polarized dusty emission core of Cygnus A
• Effect of grain size distribution and size-dependent grain heating on molecular abundances in starless and pre-stellar cores
• The radio - far infrared correlation in the faintest star forming dwarf galaxies
• Modeling Spitzer observations of VV Ser. II. an extended quantum heated nebula and a disk shadow
• On Graphene in the Interstellar Medium
• A Principal Component Analysis of polycyclic aromatic hydrocarbon emission in NGC 2023
• A bimodal dust grain distribution in the IC 434 HII region
• The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths
• Ray-tracing simulations and spectral models of X-ray radiation in dusty media
• CRIRES high-resolution near-infrared spectroscopy of diffuse interstellar band profiles. Detection of 12 new DIBs in the YJ band and the introduction of a combined ISM sight line and stellar analysis approach
• Interstellar Grains -- The 75th Anniversary
• Modelling the strongest silicate emission features of local type 1 AGN
• PAHs in Comets: An Overview
• Aliphatic hydrocarbon content of the interstellar dust
• Uncovering the Spectral Energy Distribution in Active Galaxies Using High Ionization Mid-infrared Emission Lines
• Derivation of an Analytical Approximation of the Spectrum of Spinning Dust Emission
• Dense Molecular Clumps associated with the LMC Supergiant Shells LMC 4 \& LMC 5
• Fine structure collision strengths and line ratios for [Ne V] in infrared and optical sources
• ISO far infrared observations of the high latitude cloud L1642. II. Correlated variations of far-infrared emissivity and temperature of "classical large" dust particles
• Far-Infrared Spectroscopy of Cationic Polycyclic Aromatic Hydrocarbons: Zero Kinetic Energy Photoelectron Spectroscopy of Pentacene Vaporized from Laser Desorption
• Determining the Dust Extinction of Gamma-ray Burst Host Galaxies: A Direct Method Based on Optical and X-ray Photometry
• The Mid-Infrared Colors of the ISM and Extended Sources at the Galactic Center
• Gravitational-wave constraints on the cosmic opacity at $z\sim 5$: forecast from space gravitational-wave antenna DECIGO
• Highly Embedded 8 micron Cores of Star Formation in the Spiral Arms and Filaments of 15 Nearby Disk Galaxies
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$): Detection of a dusty star-forming galaxy within the enormous Lyman $\alpha$ nebula at $z=2.3$ sheds light on its origin
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$). Mass budget, satellites spin alignment and gas infall in a massive $z\sim 3$ quasar host halo
• Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
• DZ Cha: a bona fide photoevaporating disc
• Circumstellar Structure around Evolved Stars in the Cygnus-X Star Formation Region
• IRAC Excess in Distant Star-Forming Galaxies: Tentative Evidence for the 3.3$\mu$m Polycyclic Aromatic Hydrocarbon Feature ?
• X-ray Scattering Halos from the Galactic Center: Implications for Diffuse Emission Around SgrA*
• Ultra Violet Escape Fractions from Giant Molecular Clouds During Early Cluster Formation
• Gaps in the cloud cover? Comparing extinction measures in spiral disks
• Delayed Photons from Binary Evolution Help Reionize the Universe
• Interferometric Evidence for Quantum Heated Particles in the Inner Region of Protoplanetary Disks around Herbig Stars
• Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
• ROBO: a Model and a Code for the Study of the Interstellar Medium
• The structure of the Milky Way based on unWISE 3.4$\mu$m integrated photometry
• Determination of the cosmic far-infrared background level with the ISOPHOT instrument
• A New Technique for Measuring Polycyclic Aromatic Hydrocarbon Emission in Different Environments
• Multiply charged naphthalene and its C10H8 isomers: bonding, spectroscopy and implications in AGN environments
• Cosmic Rays and Magnetic Fields in the Core and Halo of the Starburst M82: Implications for Galactic Wind Physics
• From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?
• Low-temperature optical constants of amorphous silicate dust analogues
• Interstellar Extinction and Elemental Abundances
• Millimeter Gap Contrast as a Probe for Turbulence Level in Protoplanetary Disks
• The KOSMA-$\tau$ PDR Model -- I. Recent updates to the numerical model of photo-dissociated regions
• On the missing 2175 Angstroem-bump in the Calzetti extinction curve
• [CII] $158\mu \mathrm{m}$ line emission from Orion A. I. A template for extragalactic studies?
• BAT AGN Spectroscopic Survey-XXIII. A New Mid-Infrared Diagnostic for Absorption in Active Galactic Nuclei
• Circumnuclear Star Clusters in the Galaxy Merger NGC 6240, Observed with Keck Adaptive Optics and HST
• Dust and Ionized Gas Association in E/S0 Galaxies with Dust Lanes: Clues to their Origin
• The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu
• Using cm Observations to Constrain the Abundance of Very Small Dust Grains in Galactic Cold Cores
• JINGLE, a JCMT legacy survey of dust and gas for galaxy evolution studies: II. SCUBA-2 850 μm data reduction and dust flux density catalogues
• The nuclear and integrated far-infrared emission of nearby Seyfert galaxies
• Global dust attenuation in disc galaxies: strong variation with specific star formation and stellar mass, and the importance of sample selection
• Physical conditions in three high-z H2-bearing DLAs: implications for grain size
• The Opacity of Spiral Galaxy Disks VIII: Structure of the Cold ISM
• PRIMUS: Obscured Star Formation on the Red Sequence
• Star Formation Efficiencies at Giant Molecular Cloud Scales in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
• An In-Depth View of the Mid-Infrared Properties of Point Sources and the Diffuse ISM in the SMC Giant HII Region, N66
• High Dust Depletion in Two Intervening Quasar Absorption Line Systems with the 2175-Å Extinction Bump at $z\sim 1.4$
• The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies
• The Frequency of Mid-Infrared Excess Sources in Galactic Surveys
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477
• The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
• Photoelectric heating and [CII] cooling in translucent clouds: results for cloud models based on simulations of compressible MHD turbulence
• Dust evolution processes constrained by extinction curves in nearby galaxies
• The starburst-AGN connection in the merger galaxy Mrk 938: an infrared and X-ray view
• Over-sized gas clumps in an extremely-metal-poor molecular cloud revealed by ALMA's pc-scale maps
• Relations between mid-IR dust emission and UV extinction
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• The Widespread Presence of Nanometer-size Dust Grains in the Interstellar Medium of Galaxies
• Far-infrared imaging of post-AGB stars and (proto)-planetary nebulae with the AKARI Far-Infrared Surveyor
• Intermediate-size fullerenes as degradation products of interstellar PAHs
• A Comparative Study of Knots of Star Formation in Interacting vs. Spiral Galaxies
• SOFIA/FORCAST resolves 30 - 40 um extended dust emission in nearby active galactic nuclei
• Processing of polycyclic aromatic hydrocarbons in molecular-loop regions near the Galactic center revealed by AKARI
• Toward understanding physical origin of 2175Å extinction bump in interstellar medium
• Dependence of Chemical Abundance on the Cosmic Ray Ionization Rate in IC 348
• Benchmarking Dust Emission Models in M101
• Spinning dust radiation: a review of the theory
• The dust attenuation law in $z\sim 6$ quasars
• Spitzer View of Massive Star Formation in the Tidally Stripped Magellanic Bridge
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at $z\lesssim 0.5$
• Chemical evolution of the gas in C-type shocks in dark clouds
• Universe opacity and CMB
• Discovery of a 500 pc shell in the nucleus of Centaurus A
• Outward Motion of Porous Dust Aggregates by Stellar Radiation Pressure in Protoplanetary Disks
• The fine structure line deficit in S 140
• Regulating Star Formation in Nearby Dusty Galaxies: Low Photoelectric Efficiencies in the Most Compact Systems
• Evolution of dust porosity through coagulation and shattering in the interstellar medium
• Spitzer Spectroscopy of the Galactic Supernova Remnant G292.0+1.8: Structure and Composition of the Oxygen-Rich Ejecta
• How Much Graphene in Space?
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302
• Updated Analysis of a "Dark" Galaxy and its Blue Companion in the Virgo Cloud HI 1225+01
• Modeling the Infrared Reverberation Response of the Circumnuclear Dusty Torus in AGNs: An Investigation of Torus Response Functions
• Star forming galaxies in the AKARI Deep Field South: identifications and SEDs
• Did life originate from low-temperature areas of the Universe?
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• Spitzer Observations of Dust Emission from HII Regions in the Large Magellanic Cloud
• A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy
• A machine learning potential for simulating infrared spectra of nanosilicate clusters
• Kiloparsec-scale star formation law in M81 and M101 based on AKARI far-infrared observations
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• Sub-arcsec mid-IR observations of NGC 1614: Nuclear star-formation or an intrinsically X-ray weak AGN?
• The Spitzer View of Low-Metallicity Star Formation: I. Haro 3
• Dust and Polycyclic Aromatic Hydrocarbon in the Pre-Transitional Disk around HD 169142
• Spatially-resolved Radio-to-Far-infrared SED of the Luminous Merger Remnant NGC 1614 with ALMA and VLA
• Common Correlations between 60, 100 and 140 um Intensities in the Galactic Plane and Magellanic Clouds
• The Displaced Dusty ISM of NGC 3077: Tidal Stripping in the M 81 Triplet
• Lyman-$\alpha$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
• Ages of Elliptical Galaxies: Single versus Multi Population Interpretation
• On the Unusual Depletions toward Sk 155, or What Are the Small Magellanic Cloud Dust Grains Made of?
• Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The C--D Band Strengths of Mono-Deuterated Species
• Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The C--D Band Strengths of Multi-Deuterated Species
• Ultracompact H II Regions with Extended Emission: The Complete View
• Far-infrared extinction mapping of infrared dark clouds
• ISM conditions in z~0.2 Lyman-Break Analogs
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. II. Features of Attenuation Law
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• Dust and Polycyclic Aromatic Hydrocarbon in the HD 34700 Debris Disk
• A multi-wavelength interferometric study of the massive young stellar object IRAS 13481-6124
• The dust properties and physical conditions of the interstellar medium in the LMC massive star forming complex N11
• Far-infrared dust properties in the Galaxy and the Magellanic Clouds
• Dust Extinction Law in Nearby Star-Resolved Galaxies. I. M31 Traced by Supergiants
• Variations between Dust and Gas in the Diffuse Interstellar Medium. 3. Changes in Dust Properties
• ISO observations of 3 - 200 micron emission by three dust populations in an isolated local translucent cloud
• Interstellar Extinction and Elemental Abundances: Individual Sight Lines
• Dust in AGB wind-ISM interaction regions
• DFT study of five-membered ring PAHs
• Interstellar Silicate Dust in the z=0.685 Absorber Toward TXS 0218+357
• Chemical modelling of dust-gas chemistry within AGB outflows -- II. Effect of the dust-grain size distribution
• The Physical Drivers of the Luminosity-Weighted Dust Temperatures in High-Redshift Galaxies
• High contrast and resolution near infrared photometry of the core of R136
• Constrained simulations of the Antennae Galaxies: Comparison with Herschel-PACS observations
• Interstellar dust properties of M51 from AKARI mid-infrared images
• Si isotope homogeneity of the solar nebula
• Molecular Gas Kinematics and Star Formation Properties of the Strongly-Lensed Quasar Host Galaxy RXS J1131-1231
• Effects of turbulent dust grain motion to interstellar chemistry
• Revisiting the lifetime estimate of large presolar grains in the interstellar medium
• Modeling and predicting the shape of the far-infrared to submillimeter emission in ultra-compact HII regions and cold clumps
• Evolution of PAHs in protoplanetary disks
• Cospatial Star Formation and Supermassive Black Hole Growth in $z\sim 3$ Galaxies: Evidence for In-situ Co-evolution
• Runaway stars masquerading as star formation in galactic outskirts
• Dust Extinction Law in Nearby Star-Resolved Galaxies. II. M33 Traced by Supergiants
• Dust accretion and destruction in galaxy groups and clusters
• The role of grain size in AGN torus dust models
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• Systematic errors in dust mass determinations: Insights from laboratory opacity measurements
• Observations of PAHs in the atmospheres of discs and exoplanets
• Spectropolarimetric Constraints on the Nature of Interstellar Grains
• The Spitzer View of Low-Metallicity Star Formation: II. Mrk 996, a Blue Compact Dwarf Galaxy with an Extremely Dense Nucleus
• On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump
• QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
• First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?
• Herschel/PACS Observations of the Host Galaxy of GRB 031203
• Modelling Herschel observations of infrared-dark clouds in the Hi-GAL survey
• Classification Study of WISE Infrared Sources: Identification of Candidate Asymptotic Giant Branch Stars
• On the stability of non-isothermal Bonnor-Ebert spheres. II. The effect of gas temperature on the stability
• Photon-Dominated Region Modeling of the [C I],[C II], and CO Line Emission from a Boundary in the Taurus Molecular Cloud
• Polycyclic Aromatic Hydrocarbons in Exoplanet Atmospheres I. Thermochemical Equilibrium Models
• Molecular Hydrogen Formation During Dense Interstellar Cloud Collapse
• On the Diagnostic Power of FIR/Sub-mm SED Fitting in Massive Galactic Molecular Clumps
• A resolved and asymmetric ring of PAHs within the young circumstellar disk of IRS 48
• The Long-Term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis
• A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
• JWST observations of the Horsehead photon-dominated region I. First results from multi-band near- and mid-infrared imaging
• Circumgalactic Ly$\alpha$ emission around submillimeter-bright galaxies with different quasar contributions
• Resonant infrared irradiation of CO and CH3OH interstellar ices
• Implications of Grain Size Distribution and Composition for the Correlation Between Dust Extinction and Emissivity
• The protoplanetary disc around HD 169142: circumstellar or circumbinary?
• ExoVista: A Suite of Planetary System Models for Exoplanet Studies
• Continuum Observations of M51 and M83 at 1.1 mm with AzTEC
• SPAMCART: a code for smoothed particle Monte Carlo radiative transfer
• Observations of Free-Free and Anomalous Microwave Emission from LDN 1622 with the 100 m Green Bank Telescope
• The impact of accretion heating and thermal conduction on the dead zone of protoplanetary disks
• Observations of 6 - 200 μm emission of the Ophiuchus cloud LDN 1688
• The failure of testing for cosmic opacity via the distance-duality relation
• Temperature Variations of the Cold Dust in the Triangulum Galaxy M33
• Characteristics of mid-infrared PAH emission from star-forming galaxies selected at 250 μm in the North Ecliptic Pole (NEP) field
• Properties of dust and PAHs in the hot plasma of the elliptical galaxy NGC4125 revealed with AKARI and Spitzer
• The scattering and extinction properties of nanodiamonds
• Structure Generation by Irradiation: What can GLIMPSE teach us about the ISM structure?
• Fully Sampled Maps of Ices and Silicates in Front of Cepheus A East with Spitzer
• Effects of dust abundance on the far-infrared colours of blue compact dwarf galaxies
• On Carbon Nanotubes in the Interstellar Medium
• Molecular gas budget and characterization of intermediate-mass star-forming galaxies at $z\approx 2-3$
• Impact of Dust on Spectral Distortion Measurements of the Cosmic Microwave Background
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• Scattered H-alpha emission from a large translucent cloud G294-24
• Mid-infrared imaging and modelling of the dust shell around post-AGB star HD 187885 (IRAS 19500-1709)
• Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
• Are the Formation and Abundances of Metal-Poor Stars the Result of Dust Dynamics?
• Spectral energy distributions of dust and PAHs based on the evolution of grain size distribution in galaxies
• Feasibility of detecting shadows in disks induced by infall
• Kathryns Wheel: A spectacular galaxy collision discovered in the Galactic neighbourhood
• Nanodust in the Interstellar Medium in Comparison to the Solar System
• The HI supershell GS 118+01-44 and its role in the interstellar medium
• Extraplanar gas in Edge-on Galaxies traced by SOFIA observations of [C II]
• The physical state of selected cold clumps
• Is the mm/submm dust polarization a robust tracer of the magnetic field topology in protostellar envelopes? A model exploration
• Evolution of dust grain size distribution and grain porosity in galaxies
• Limits on Intergalactic Dust During Reionization
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• Restructuring and destruction of hydrocarbon dust in the interstellar medium
• The Distortion of the Cosmic Microwave Background Spectrum Due to Intergalactic Dust
• Dust properties along anomalous extinction sightlines. II. Studying extinction curves with dust models
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Extinction calculations of multi-sphere polycrystalline graphitic clusters - A comparison with the 2175 AA peak and between a rigorous solution and discrete-dipole approximations
• Dense Gas and Star Formation in Nearby Infrared Bright Galaxies: APEX survey of HCN and HCO+ J=2-1
• Linear dust polarization during the embedded phase of protostar formation
• Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
• The edge-on disk Tau042021: icy grains at high altitudes and a wind containing astronomical PAHs
• Dust Models for the Extinction of Type IIn Supernova SN 2010jl
• The complex infrared dust continuum emission of NGC1068: ground-based N- and Q-band spectroscopy and new radiative transfer models
• Near- to mid-Infrared Observations of Galaxy Mergers: NGC2782 and NGC7727
• Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
• Dissecting the central regions of OH 231.8 + 4.2 with ALMA: a salty rotating disk at the base of a young bipolar outflow
• Modeling IR Spectral Energy Distributions: A Pilot Study of Starburst Parameters and Silicate Absorption Curves for Some GOALS Galaxies
• Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
• SOFIA/HAWC+ observations of the Crab Nebula: dust properties from polarised emission
• A Multiwavelength View of Star Formation in Interacting Galaxies in the Pavo Group
• LABOCA and MAMBO-2 imaging of the dust ring of the Sombrero galaxy (NGC 4594)
• Missing dust signature in the cosmic microwave background
• Correlation between UV resilience and wavelength of narrow DIBs
• Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Optical and Infrared Imaging and Spectroscopy of the Multiple-Shell Planetary Nebula NGC 6369
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• Radiative Transfer Modeling of An SN 1987A Light Echo$-$AT2019xis
• Dust Extinction towards the Type Ia Supernova 2012cu in NGC 4772
• Grain Physics and Rosseland Mean Opacities
• The 2175 Angstrom Interstellar Extinction Bump: Is the Wavelength Variable?
• The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities
• Dark Dust III: The high-quality single-cloud reddening curve sample. Scrutinizing extinction curves in the Milky Way
• Dust Emission from Evolved and Unevolved HII Regions in the Large Magellanic Cloud
• Thermal emission from the amorphous dust: An alternative possibility of the origin of the anomalous microwave emission
• Spinning Dust Emission from Wobbling Grains: Important Physical Effects and Implications
• ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion
• Dust emission at 8-mic and 24-mic as Diagnostics of HII Region Radiative Transfer
• Modelling galaxy spectra in presence of interstellar dust-III. From nearby galaxies to the distant Universe
• Importance of far-infrared mapping in a spiral galaxy: AKARI observation of M81
• Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
• Spectroscopic infrared extinction mapping as a probe of grain growth in IRDCs
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• Extinction Laws toward Stellar Sources within a Dusty Circimstellar Medium and Implications for Type Ia Supernovae
• Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
• Observational signatures of the dust size evolution in isolated galaxy simulations
• The incidence of mid-infrared excesses in G and K giants
• Enhanced dust emissivity power-law index along the western H$\alpha$ filament of NGC 1569
• The role of molecular gas in the nuclear regions of IRAS 00183-7111. ALMA and X-ray investigations of an ultraluminous infrared galaxy
• Ultraviolet extinction properties of the 30 Dor Nebula and interpreting observations of starburst clusters
• Effects of rotational disruption on the evolution of grain size distribution in galaxies
• A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
• Observing the Earliest Stages of Star Formation in Galaxies: 8 micron Cores in Three Edge-on Disks
• A probable Keplerian disk feeding an optically revealed massive young star
• Spatially resolving polycyclic aromatic hydrocarbons in Herbig Ae disks with VISIR-NEAR at the VLT
• Searching for a cometary belt around Trappist-1 with ALMA
• UV-FIR SED modeling of AGN in IR-luminous galaxies up to z~2.5: Understanding the effects of torus models
• Spatially resolved dust emission of extremely metal poor galaxies
• Spatial distribution of the aromatic and aliphatic carbonaceous nano-grain features in the protoplanetary disk around HD 100546
• The Physical Characteristics of Interstellar Medium in NGC 3665 with Herschel Observations
• Molecular Gas Heating and Modified Dust Properties in Active Galaxies: Growing Black Holes or Tidal Shocks?
• Star Formation and the Interstellar Medium In Nearby Tidal Streams (SAINTS): Spitzer Mid-infrared Spectroscopy and Imaging of Intergalactic Star-forming Objects
• 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
• Modelling Grain Rotational Disruption by Radiative Torques and Extinction of Active Galactic Nuclei
• A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements
• Effect of surface H${}_2$ on molecular hydrogen formation on interstellar grains
• Dust in the Local Group
• Search for signatures of dust in the Pluto-Charon system using Herschel/PACS observations
• A deep-learning approach to the 3D reconstruction of dust density and temperature in star-forming regions
• The rotational disruption of porous dust aggregates from ab-initio kinematic calculations
• Environmental Dependence of Star Formation Law in the Disk and Center of IC 342
• Signature of outflows in strong MgII absorbers in quasar sightlines
• Five new hot-Jupiter transits investigated with Swift-UVOT
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• Cosmic Biology in Perspective
• Carbon 'fluffy' aggregates produced by helium - hydrocarbon high pressure plasmas as analogs to interstellar dust
• Mid-IR FORCAST/SOFIA Observations of M82
• Detectability of Polycyclic Aromatic Hydrocarbons in the Atmosphere of WASP-6 b with JWST NIRSpec PRISM
• What causes the ultraviolet extinction bump at the cosmic dawn?
• On the Absorption Properties of Metallic Needles
• A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
• Comparing Infrared Star-Formation Rate Indicators with Optically-Derived Quantities
• Recent Results of Solid-State Spectroscopy
• Dust Properties of Clumpy Disc Galaxies at z~1.3 with Herschel-SPIRE
• Detection of an ultra-bright submillimeter galaxy behind the Small Magellanic Cloud
• Impact of dust diffusion on the rim shape of protoplanetary disks
• The Impact of Inclination-dependent Attenuation on Ultraviolet Star Formation Rate Tracers
• Dust SEDs in Milky Way-like galaxies in the IllustrisTNG simulations based on the evolution of grain size distribution
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Dust Mass Associated with the Supernova Remnant IC 443 when Emission Meets Extinction
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• The Cosmic-Ray Induced Sputtering Process On Icy Grains
• [CII] emission properties of the massive star-forming region RCW36 in a filamentary molecular cloud
• Revisiting the Local Interstellar Radiation Field using Gaia DR3
• The Radial Profile of Dust Grain Size in the Protoplanetary Disk of DS Tau
• New Mid-Infrared Imaging Constraints on Companions and Protoplanetary Disks around six Young Stars
• On planet formation around supermassive black holes and the grain disruption barriers by radiative torques
• The Wyoming Survey for H-alpha. III. A Multi-wavelength Look at Attenuation by Dust in Galaxies out to z~0.4
• Global Spectral Energy Distributions of the Large Magellanic Cloud with Interstellar Dust
• Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z~3.3
• UV/Optical/IR Color Sequences Along the Tidal Ring/Arm of Arp 107
• The impact of cosmic ray feedback during the epoch of reionisation
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• Mid-infrared extinction toward the Galactic center
• Synthetic observations of protostellar multiple systems
• Processing of hydrocarbon dust in star-forming galaxies revealed with AKARI
• A Massive Gas Outflow Outside the Line-of-Sight: Imaging Polarimetry of the Blue Excess Hot Dust Obscured Galaxy W0204-0506
• Molecules with ALMA at Planet-forming Scales (MAPS) XVII: Determining the 2D Thermal Structure of the HD 163296 Disk
• SPHEREx: Aromatics, Aliphatics and PAH Size across the Iris Nebula
• NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• Magnetism of Fullerene C60 Compared with Graphene Molecule by DFT Calculation, Laboratory Experiment and Astronomical Observation
• The hydrogen Balmer lines and jump in absorption in accretion disc modeling -- an ultraviolet-optical spectral analysis of the dwarf novae UZ Serpentis and CY Lyrae
• Modelling the SEDs of spiral galaxies
• A simple model of dust extinction in gamma-ray burst host galaxies
• Estimation of high-resolution dust column density maps: Empirical model fits
• GATOS XI : Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI
• Outflows from starburst galaxies with various driving mechanisms and their X-ray properties
• On the band-to-continuum intensity ratio in the infrared spectra of interstellar carbonaceous dust
• Time-Varying Extinction, Polarization, and Colors of Type Ia Supernovae due to Rotational Disruption of Dust Grains
• Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
• The Binding Energies of Atoms on Amorphous Silicate Dust: A Computational Study
• Polycyclic aromatic hydrocarbon (PAH) abundances in the disk around T Chamaeleontis (T Cha): PAH sizes, ionization fraction, and mass during JWST observations
• A systematic study on the properties of aromatic and aliphatic hydrocarbon dust in active galactic nuclei with AKARI near-infrared spectroscopy
• MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
• Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
• Interstellar Grains: Effect of Inclusions on Extinction
• Effects of grain temperature distribution on organic protostellar envelope chemistry
• The Large Magellanic Cloud: A power spectral analysis of Spitzer images
• Dense Star-forming Gas and Dust in the Magellanic Clouds
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Constraining the Metallicities of Damped Ly$\alpha$ Systems Using Extinction Curves
• Modeling Long-Wavelength Amorphous Dust Emission Based on the Physically Motivated Soft-Potential Model
• Better Alternative to "Astronomical Silicate": Laboratory-Based Optical Functions of Chondritic/Solar Abundance Glass With Application to HD161796
• A Semi-Empirical Model of the Infrared Emission from Galaxies
• Exploring the 100 au Scale Structure of the Protobinary System NGC 2264 CMM3 with ALMA
• An Improved Pair Method to Probe the Dust Extinction Law
• Analytic formulas for frequency and size dependence of absorption and scattering efficiencies of astronomical polycyclic aromatic hydrocarbons
• Studying the spectral properties of Active Galactic Nuclei in the JWST era
• Void defect induced magnetism and structure change of carbon material-3, Polycyclic aromatic hydrocarbon
• The role of young and evolved stars in the heating of dust in local galaxies
• What is the amount of baryonic dark matter in galaxies?
• MINDS survey of silicates in T Tauri disks: Correlation between dust and gas
• Optical constants of Ih, Ic, and amorphous H${}_2$O ices in the THz and IR ranges
• A Detailed Analysis of Intermediate-scale Structure in Optical Extinction Curves: Expanded Census and Two-family Classification