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

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• Forces on Dust Grains Exposed to Anisotropic Interstellar Radiation Fields
• Radiative Transfer Analysis of Far-UV Background Observations Obtained with the Far-Ultraviolet Space Telescope (FAUST)
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• The nature of dust in compact Galactic planetary nebulae from Spitzer spectra
• Dust models post-Planck: constraining the far-infrared opacity of dust in the diffuse interstellar medium
• Spectacular Spitzer images of the Trifid Nebula: Protostars in a young, massive-star-forming region
• Quantifying non-star formation associated 8um dust emission in NGC 628
• Modeling the Infrared Emission from the HR 4796A Disk
• Low-temperature MIR to submillimeter mass absorption coefficient of interstellar dust analogues II: Mg and Fe-rich amorphous silicates
• The Dust & Gas Properties of M83
• Inferring the Redshift Distribution of the Cosmic Infrared Background
• AGN-driven outflows and the formation of Ly$\alpha$ nebulae around high-z quasars
• Laboratory photo-chemistry of pyrene clusters: an efficient way to form large PAHs
• Spitzer Mapping of PAHs and H2 in Photodissociation Regions
• Nearby early-type galaxies with ionized gas VI. The Spitzer-IRS view
• Deciphering Lyman-$\alpha$ Emission Deep into the Epoch of Reionisation
• H2 formation on PAHs in photodissociation regions: a high-temperature pathway to molecular hydrogen
• The Mid-Infrared Extinction Law and its Variation in the Coalsack Nebula
• Testing Star Formation Laws in a Starburst Galaxy At Redshift 3 Resolved with ALMA
• The Molecular Interstellar Medium of the Local Group Dwarf NGC6822
• Simulating the diversity of shapes of the Lyman-$\alpha$ line
• Sculpting the disk around T Cha: an interferometric view
• On the Morphology and Chemical Composition of the HR 4796A Debris Disk
• Unusual PAH Emission in Nearby Early-Type Galaxies: A Signature of an Intermediate Age Stellar Population?
• T-carbon: experiments, properties, derivatives and potential applications
• Search for corannulene (C20H10) in the Red Rectangle
• The Circumstellar Environment of R Coronae Borealis: White Dwarf Merger or Final Helium Shell Flash?
• Probing the Nuclear and Circumnuclear Activity of NGC1365 in the Infrared
• The Mipsgal View of Supernova Remnants in the Galactic Plane
• Modelling galaxy spectra in presence of interstellar dust. I. The model of ISM and the library of dusty SSPs
• 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
• 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
• Spitzer and JCMT Observations of the Active Galactic Nucleus in the Sombrero Galaxy (NGC 4594)
• A multi-wavelength investigation of RCW175: an HII region harboring spinning dust emission
• Constraint on the Polarization of Electric Dipole Emission from Spinning Dust
• Simulating radiative feedback and star cluster formation in GMCs: I. Dependence on gravitational boundedness
• Molecular gas properties of a lensed star-forming galaxy at z~3.6: a case study
• Star formation around the HII region Sh2-235
• PHANGS-JWST First Results: Tracing the Diffuse ISM with JWST Imaging of Polycyclic Aromatic Hydrocarbon Emission in Nearby Galaxies
• Probing the Protostellar Envelope around L1157: the Dust and Gas Connection
• A Dust spectral energy distribution model with hierarchical Bayesian inference. I. Formalism & benchmarking
• Simulations of protostellar collapse using multigroup radiation hydrodynamics. I. The first collapse
• What produces the far-infrared/submm emission in the most luminous QSOs?
• The Spectrum of Integrated Millimeter Flux of the Magellanic Clouds and 30-Doradus from TopHat and DIRBE Data
• 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
• NOEMA redshift measurements of bright Herschel galaxies
• Spitzer Analysis of HII Region Complexes in the Magellanic Clouds: Determining a Suitable Monochromatic Obscured Star Formation Indicator
• Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
• Full SED fitting with the KOSMA-τ PDR code - I. Dust modelling
• Physical properties of the ambient medium and of dense cores in the Perseus star-forming region derived from Herschel Gould Belt Survey observations
• Variation of the extinction law in the Trifid nebula
• Modeling Mid-Infrared Diagnostics of Obscured Quasars and Starbursts
• Mid-Infrared Spectroscopy of Infrared Luminous Galaxies with Sub-Arcsecond Resolution
• Evolution of the extinction curves in galaxies
• Infrared Spectral Energy Distribution Model for Extremely Young Galaxies
• Interstellar extinction and interstellar polarization: old and new models
• Spatially Resolved 3 micron Spectroscopy of Elias 1: Origin of Diamonds in Protoplanetary Disks
• The Interstellar Oxygen Crisis, or Where Have All the Oxygen Atoms Gone?
• Effects of grain growth mechanisms on the extinction curve and the metal depletion in the interstellar medium
• Probing the Role of Carbon in the Interstellar Ultraviolet Extinction
• The Spatial Distribution of Dust and Stellar Emission of the Magellanic Clouds
• The Extreme Star Formation Activity of Arp299 Revealed by Spitzer IRS Spectral Mapping
• Sensitivity of PDR Calculations to Microphysical Details
• Planck intermediate results. XXV. The Andromeda Galaxy as seen by Planck
• The evolution of actively star forming galaxies in the mid infrared
• Extinction curve template for intrinsically reddened quasars
• A Tale of Two Mysteries in Interstellar Astrophysics: The 2175 Angstrom Extinction Bump and Diffuse Interstellar Bands
• Constraining dust formation in high-redshift young galaxies
• High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030
• The Carriers of the "Unidentified" Infrared Emission Features: Clues from Polycyclic Aromatic Hydrocarbons with Aliphatic Sidegroups
• Simulating radiative feedback and star cluster formation in GMCs: II. Mass dependence of cloud destruction and cluster properties
• Properties of Starless and Prestellar Cores in Taurus Revealed by Herschel SPIRE/PACS Imaging
• Spinning dust emission from ultrasmall silicates: emissivity and polarization spectrum
• Star formation histories, extinction, and dust properties of strongly lensed z~1.5-3 star-forming galaxies from the Herschel Lensing Survey
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• Extinction Correction for Type Ia Supernova Rates. I. The Model
• The Herschel Virgo cluster survey: V. Star-forming dwarf galaxies - dust in metal-poor environments
• Gas and Star Formation in the Circinus Galaxy
• Polycyclic aromatic hydrocarbon (PAH) luminous galaxies at z~1
• Comprehensive Gas Characterization of a $z=2.5$ Protocluster: A Cluster Core Caught in the Beginning of Virialization?
• On The Gas Temperature of Molecular Cloud Cores
• The Spatially Resolved Dust-to-Metals Ratio in M101
• Far-infrared Observations of the Very Low-Luminosity Embedded Source L1521F-IRS in the Taurus Star-Forming Region
• Observing Extended Sources with the \Herschel SPIRE Fourier Transform Spectrometer
• Silicate Composition of the Interstellar Medium
• Mitigating Complex Dust Foregrounds in Future CMB Polarization Experiments
• On the Flux of Extra-Solar Dust in Earth's Atmosphere
• Spitzer characterisation of dust in an anomalous emission region: the Perseus cloud
• Candidate Water Vapor Lines to Locate the H${}_2$O Snowline through High-Dispersion Spectroscopic Observations I. The Case of a T Tauri Star
• Supernovae and AGN driven galactic outflows
• On the Measurement of Elemental Abundance Ratios in Inner Galaxy H II Regions
• The X-Ray Scattering Halo Around Nova Cygni 1992: Testing a Model for Interstellar Dust
• Silicate Emission in the Spitzer IRS spectrum of FSC 10214+4724
• The Mystery of Unidentified Infrared Emission Bands
• The roles of star formation and AGN activity of IRS sources in the HerMES fields
• Self-consistent modelling of aromatic dust species and extinction curves in galaxy evolution
• Warm Dust and Spatially Variable PAH Emission in the Dwarf Starburst Galaxy NGC 1705
• 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
• Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk
• 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
• A chemical model for the interstellar medium in galaxies
• Towards Detecting The 2175-Å Dust Feature Associated With Strong High Redshift Mg ßII Absorption Lines
• Observations of Cold Dust in Nearby Elliptical Galaxies
• Unidentified Infrared Bands in the Interstellar Medium across the Galaxy
• The gas-to-dust mass ratio of Centaurus A as seen by Herschel
• VLT Spectropolarimetry of the optical transient in NGC300. Evidence for asymmetry in the circumstellar dust
• Dissecting the origin of the submillimeter emission in nearby galaxies with Herschel and LABOCA
• Dual-Wavelength ALMA Observations of Dust Rings in Protoplanetary Disks
• X-Ray Scattering by Nonspherical Grains. I. Oblate Spheroids
• Variations between Dust and Gas in the Diffuse Interstellar Medium
• Multi-phase outflows in post starburst E+A galaxies -- I. General sample properties and the prevalence of obscured starbursts
• X-ray radiative transfer in full 3D with SKIRT
• Silicate Dust in Active Galactic Nuclei
• The fate of the Antennae galaxies
• Star-forming accretion flows and the low luminosity nuclei of giant elliptical galaxies
• Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
• Lyα emission from galaxies in the Epoch of Reionization
• The physical and chemical structure of Sagittarius B2 -- V. Non-thermal emission in the envelope of Sgr B2
• Mid--IR emission of galaxies in the Virgo cluster: II. Integrated properties
• 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
• The Galactic Census of High- and Medium-mass Protostars. II. Luminosities and Evolutionary States of a Complete Sample of Dense Gas Clumps
• 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?
• X-ray radiative transfer in protoplanetary disks - The role of dust and X-ray background fields
• Examining the class B-to-A shift of the 7.7 $\mu$m PAH band with the NASA Ames PAH IR Spectroscopic Database
• Time-Dependent, Multifluid, Magnetohydrodynamic Shock Waves with Grain Dynamics I. Formulation and Numerical Tests
• Mapping the interstellar medium in galaxies with Herschel/SPIRE
• Evaporation of Low-Mass Planet Atmospheres: Multidimensional Hydrodynamics with Consistent Thermochemistry
• 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
• Modeling the Infrared Interstellar Extinction
• On the stability of non-isothermal Bonnor-Ebert spheres
• Can Fluffy Dust Alleviate the "Subsolar" Interstellar Abundance Problem?
• The thermal dust emission in the N158-N159-N160 (LMC) star forming complex mapped by Spitzer, Herschel and LABOCA
• First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
• Spatial Distribution of Dust Grains within H II Regions
• Spatially Resolved Spitzer Spectroscopy of the Starburst Nucleus in NGC 5253
• Dust enshrouded star-forming activity in Arp 299
• Star-formation histories of local luminous infrared galaxies
• Herschel-ATLAS: Correlations between Dust and Gas in Local Submm-Selected Galaxies
• Mid-Infrared Spectropolarimetric Constraints on the Core-Mantle Interstellar Dust Model
• The Origin of the 4.5 micron Excess from Dwarf Galaxies
• Spiral Structure and Differential Dust Size Distribution in the LkHa 330 Disk
• PAH Spectroscopy from 1-5 $\mu$m
• High-resolution mapping of interstellar clouds with near-infrared scattered light
• The Pseudo-zodi Problem for Edge-on Planetary Systems
• Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains
• Probing the Interstellar Dust towards the Galactic Centre: Dust Scattering Halo around AX J1745.6-2901
• 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
• 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
• The cosmic carbon footprint of massive stars stripped in binary systems
• GRASIL-3D: an Implemention of Dust Effects in the SEDs of Simulated Galaxies
• Tracing the ISM magnetic field morphology: The potential of multi-wavelength polarization measurements
• L1495 Revisited: A PPMAP View of a Star-Forming Filament
• The Star Formation History of the Virgo early-type galaxy NGC4435: the Spitzer Mid Infrared view
• VLT/X-shooter GRBs: Individual extinction curves of star-forming regions
• Mapping the Escape Fraction of Ionizing Photons Using Resolved Stars: A Much Higher Escape Fraction for NGC 4214
• 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
• Evolution of dust and molecular hydrogen in the Magellanic System
• Quantifying the (X/peanut)-shaped Structure of the Milky Way - New Constraints on the Bar Geometry
• Shiva: the dust destruction model
• Predictions of polarized dust emission from interstellar clouds: spatial variations in the efficiency of radiative torque alignment
• Herschel and SCUBA-2 observations of dust emission in a sample of Planck cold clumps
• 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
• Molecular Hydrogen in the Ionized Region of Planetary Nebulae
• Multiband Polarimetric Imaging of HR 4796A with the Gemini Planet Imager
• Some Stars are Totally Metal: A New Mechanism Driving Dust Across Star-Forming Clouds, and Consequences for Planets, Stars, and 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
• Near-Infrared Integral Field Spectroscopy of Star-Forming Galaxies
• Spitzer Observations of Cold Dust Galaxies
• Simulating the UV Escape Fractions from Molecular Cloud Populations in Star-forming Dwarf and Spiral Galaxies
• Extra-Nuclear Starbursts: Young Luminous Hinge Clumps in Interacting Galaxies
• Through the magnifying glass: ALMA acute viewing of the intricate nebular architecture of OH231.8+4.2
• X-ray versus Optical Observations of Active Galactic Nuclei: Evidence for Large Grains?
• Diffuse Interstellar Bands and the Ultraviolet Extinction Curves: The Missing Link Revisited
• Far-Infrared Properties of Blue Compact Dwarf Galaxies Observed with AKARI/Far-Infrared Surveyor (FIS)
• GALEX UV properties of the polar ring galaxy MCG-05-07-001 and the shell galaxies NGC 1210 and NGC 5329
• Mid-infrared spectroscopy of Spitzer-selected ultra-luminous starbursts at z~2
• On the origin of M81 group extended dust emission
• EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function
• A Cometary Bow Shock and Mid-Infrared Emission Variations Revealed in Spitzer Observations of HD 34078 and IC 405
• Stellar Populations and the Star Formation Histories of LSB Galaxies: IV Spitzer Surface Photometry of LSB Galaxies
• The Bright Extragalactic ALMA Redshift Survey (BEARS) II: Millimetre photometry of gravitational lens candidates
• The 3.3 micron PAH Emission as a Star Formation Rate Indicator
• A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures Across Cosmic Time
• The Balloon-Borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 10 deg^2 Survey of Star Formation in Cygnus X
• Extended Emission by Dust in the Dwarf Galaxy UGC 10445
• Identification of Main Sequence Stars with Mid-Infrared Excesses Using GLIMPSE: Beta-Pictoris Analogs?
• A Corona Australis cloud filament seen in NIR scattered light I. Comparison with extinction of background stars
• Dust emissivity and absorption cross section in DustPedia late-type galaxies
• The Dust in M31
• Probing Cosmic Dust of the Early Universe through High-Redshift Gamma-Ray Bursts
• Structure of the interstellar medium around Cas A
• Extremely massive young clusters in NGC1365
• Lanthanides or dust in kilonovae: lessons learned from GW170817
• Constraining the ISM properties of the Cloverleaf quasar host galaxy with Herschel spectroscopy
• The Mid-Infrared [SIV]/[NeII] versus [NeIII]/[NeII] Correlation
• Modelling galaxy spectra in presence of interstellar dust. II. From the UV to the far infrared
• Infrared Emission from Intracluster Dust Grains and Constraints on Dust Properties
• Uncovering Red and Dusty Ultraluminous X-ray Sources with Spitzer
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• The Herschel Virgo Cluster Survey. XVIII. Star-forming dwarf galaxies in a cluster environment
• Millimeter and Submillimeter Excess Emission in M33 revealed by Planck and LABOCA
• 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
• Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star Forming Galaxies at z $\sim$ 3
• Shattering by turbulence as a production source of very small grains
• Cosmic Needles versus Cosmic Microwave Background Radiation
• An Empirical Decomposition of Near-IR Emission into Galactic and Extragalactic Components
• 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
• Dust Destruction by Charging: A Possible Origin of Grey Extinction Curves of Active Galactic Nuclei
• LABOCA observations of giant molecular clouds in the south west region of the Small Magellanic Cloud
• Interstellar dust along the line of sight of GX 3+1
• 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
• An embedded active nucleus in the OH megamaser galaxy IRAS16399-0937
• Absorption by Spinning Dust: a Contaminant for High-Redshift 21 cm Observations
• Composite Interstellar Grains
• Light Echoes of Transients and Variables in the Local Universe
• Galactic Center Extinction: Evidence for Metallic Needles in the General Interstellar Medium
• Radiative transfer of ionizing radiation through gas and dust: stellar source case
• Isentropic thermal instability in atomic surface layers of photodissociation regions
• On the Aliphatic versus Aromatic Content of the Carriers of the "Unidentified" Infrared Emission Features
• Panspermia in a Milky Way-like Galaxy
• The impact of the Star Formation Histories on the SFR-M${}_{\ast }$ relation at z$\ge$2
• Photoelectric Heating and [CII] Cooling of High Galactic Latitude Translucent Clouds
• On Buckyonions as an Interstellar Grain Component
• Determination of the far-infrared dust opacity in a prestellar core
• [O I] 63 micron Emission from High and Low Luminosity AGN Galaxies
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• Extinction in the 11.2 micron PAH band and the low L_11.2/L_IR in ULIRGs
• Far-Infrared detection of neutral atomic oxygen toward the Horsehead Nebula
• Interstellar Silicon Depletion and the Ultraviolet Extinction
• Effect of grain size distribution and size-dependent grain heating on molecular abundances in starless and pre-stellar cores
• The highly polarized dusty emission core of Cygnus A
• The post-Herschel view of intrinsic AGN emission: constructing templates for galaxy and AGN emission at IR wavelengths
• 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
• On Graphene in the Interstellar Medium
• A Principal Component Analysis of polycyclic aromatic hydrocarbon emission in NGC 2023
• Submillimeter imaging of the Galactic Center starburst Sgr B2. Warm molecular, atomic, and ionized gas far from massive star-forming cores
• A bimodal dust grain distribution in the IC 434 HII region
• 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
• Ray-tracing simulations and spectral models of X-ray radiation in dusty media
• Uncovering the Spectral Energy Distribution in Active Galaxies Using High Ionization Mid-infrared Emission Lines
• Aliphatic hydrocarbon content of the interstellar dust
• 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
• Modelling the strongest silicate emission features of local type 1 AGN
• 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
• PAHs in Comets: An Overview
• ISO far infrared observations of the high latitude cloud L1642. II. Correlated variations of far-infrared emissivity and temperature of "classical large" dust particles
• Fine structure collision strengths and line ratios for [Ne V] in infrared and optical sources
• Dense Molecular Clumps associated with the LMC Supergiant Shells LMC 4 \& LMC 5
• Interstellar Grains -- The 75th Anniversary
• Derivation of an Analytical Approximation of the Spectrum of Spinning Dust Emission
• DZ Cha: a bona fide photoevaporating disc
• X-ray Scattering Halos from the Galactic Center: Implications for Diffuse Emission Around SgrA*
• Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
• Circumstellar Structure around Evolved Stars in the Cygnus-X Star Formation Region
• 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
• The Mid-Infrared Colors of the ISM and Extended Sources at the Galactic Center
• 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
• IRAC Excess in Distant Star-Forming Galaxies: Tentative Evidence for the 3.3$\mu$m Polycyclic Aromatic Hydrocarbon Feature ?
• 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
• Determination of the cosmic far-infrared background level with the ISOPHOT instrument
• Interferometric Evidence for Quantum Heated Particles in the Inner Region of Protoplanetary Disks around Herbig Stars
• Gaps in the cloud cover? Comparing extinction measures in spiral disks
• Investigation of the Origin of the Anomalous Microwave Emission in Lambda Orionis
• Delayed Photons from Binary Evolution Help Reionize the Universe
• A New Technique for Measuring Polycyclic Aromatic Hydrocarbon Emission in Different Environments
• Ultra Violet Escape Fractions from Giant Molecular Clouds During Early Cluster Formation
• The KOSMA-$\tau$ PDR Model -- I. Recent updates to the numerical model of photo-dissociated regions
• Interstellar Extinction and Elemental Abundances
• The structure of the Milky Way based on unWISE 3.4$\mu$m integrated photometry
• Cosmic Rays and Magnetic Fields in the Core and Halo of the Starburst M82: Implications for Galactic Wind Physics
• [CII] $158\mu \mathrm{m}$ line emission from Orion A. I. A template for extragalactic studies?
• From flux to dust mass: Does the grain-temperature distribution matter for estimates of cold dust masses in supernova remnants?
• Multiply charged naphthalene and its C10H8 isomers: bonding, spectroscopy and implications in AGN environments
• ROBO: a Model and a Code for the Study of the Interstellar Medium
• On the missing 2175 Angstroem-bump in the Calzetti extinction curve
• Low-temperature optical constants of amorphous silicate dust analogues
• Millimeter Gap Contrast as a Probe for Turbulence Level in Protoplanetary Disks
• The effect of active galactic nuclei on the cold interstellar medium in distant star-forming galaxies
• The Extinction Properties of and Distance to the Highly Reddened Type Ia Supernova SN 2012cu
• 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
• The nuclear and integrated far-infrared emission of nearby Seyfert galaxies
• 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
• Star Formation Efficiencies at Giant Molecular Cloud Scales in the Molecular Disk of the Elliptical Galaxy NGC 5128 (Centaurus A)
• Global dust attenuation in disc galaxies: strong variation with specific star formation and stellar mass, and the importance of sample selection
• The Frequency of Mid-Infrared Excess Sources in Galactic Surveys
• 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
• An In-Depth View of the Mid-Infrared Properties of Point Sources and the Diffuse ISM in the SMC Giant HII Region, N66
• Absence of nuclear polycyclic aromatic hydrocarbon emission from a compact starburst: The case of the type-2 quasar Mrk 477
• Using cm Observations to Constrain the Abundance of Very Small Dust Grains in Galactic Cold Cores
• The Spectral Energy Distribution of Self-gravitating Interstellar Clouds I. Spheres
• Non-Universal Stellar Initial Mass Functions: Large Uncertainties in Star Formation Rates at $z\approx 2-4$ and Other Astrophysical Probes
• Photoelectric heating and [CII] cooling in translucent clouds: results for cloud models based on simulations of compressible MHD turbulence
• High Dust Depletion in Two Intervening Quasar Absorption Line Systems with the 2175-Å Extinction Bump at $z\sim 1.4$
• Dust and Ionized Gas Association in E/S0 Galaxies with Dust Lanes: Clues to their Origin
• PRIMUS: Obscured Star Formation on the Red Sequence
• Dust evolution processes constrained by extinction curves in nearby galaxies
• Spinning dust radiation: a review of the theory
• Dependence of Chemical Abundance on the Cosmic Ray Ionization Rate in IC 348
• Modelling the dusty universe II: The clustering of submillimetre-selected galaxies
• A Comparative Study of Knots of Star Formation in Interacting vs. Spiral Galaxies
• Toward understanding physical origin of 2175Å extinction bump in interstellar medium
• The starburst-AGN connection in the merger galaxy Mrk 938: an infrared and X-ray view
• Processing of polycyclic aromatic hydrocarbons in molecular-loop regions near the Galactic center revealed by AKARI
• The Widespread Presence of Nanometer-size Dust Grains in the Interstellar Medium of Galaxies
• Intermediate-size fullerenes as degradation products of interstellar PAHs
• Far-infrared imaging of post-AGB stars and (proto)-planetary nebulae with the AKARI Far-Infrared Surveyor
• The dust attenuation law in $z\sim 6$ quasars
• SOFIA/FORCAST resolves 30 - 40 um extended dust emission in nearby active galactic nuclei
• Relations between mid-IR dust emission and UV extinction
• Over-sized gas clumps in an extremely-metal-poor molecular cloud revealed by ALMA's pc-scale maps
• Benchmarking Dust Emission Models in M101
• TODDLERS: A new UV-mm emission library for star-forming regions. 1. Integration with SKIRT and public release
• Discovery of a 500 pc shell in the nucleus of Centaurus A
• Measuring the average molecular gas content of star-forming galaxies at $z=3-4$
• Outward Motion of Porous Dust Aggregates by Stellar Radiation Pressure in Protoplanetary Disks
• An X-ray study of the SNR G344.7-0.1 and the central object CXOU J170357.8-414302
• Universe opacity and CMB
• Chemical evolution of the gas in C-type shocks in dark clouds
• 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
• AKARI mid-infrared slitless spectroscopic survey of star-forming galaxies at $z\lesssim 0.5$
• How Much Graphene in Space?
• Modelling the dusty universe I: Introducing the artificial neural network and first applications to luminosity and colour distributions
• Spitzer Spectroscopy of the Galactic Supernova Remnant G292.0+1.8: Structure and Composition of the Oxygen-Rich Ejecta
• Spitzer View of Massive Star Formation in the Tidally Stripped Magellanic Bridge
• The fine structure line deficit in S 140
• Lyman-$\alpha$ feedback prevails at Cosmic Dawn: Implications for the first galaxies, stars, and star clusters
• Updated Analysis of a "Dark" Galaxy and its Blue Companion in the Virgo Cloud HI 1225+01
• Did life originate from low-temperature areas of the Universe?
• Modeling the Infrared Reverberation Response of the Circumnuclear Dusty Torus in AGNs: An Investigation of Torus Response Functions
• Common Correlations between 60, 100 and 140 um Intensities in the Galactic Plane and Magellanic Clouds
• Kiloparsec-scale star formation law in M81 and M101 based on AKARI far-infrared observations
• On the Unusual Depletions toward Sk 155, or What Are the Small Magellanic Cloud Dust Grains Made of?
• A machine learning potential for simulating infrared spectra of nanosilicate clusters
• Spitzer Observations of Dust Emission from HII Regions in the Large Magellanic Cloud
• 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
• Spatially-resolved Radio-to-Far-infrared SED of the Luminous Merger Remnant NGC 1614 with ALMA and VLA
• Dust and Polycyclic Aromatic Hydrocarbon in the Pre-Transitional Disk around HD 169142
• Ages of Elliptical Galaxies: Single versus Multi Population Interpretation
• Star forming galaxies in the AKARI Deep Field South: identifications and SEDs
• A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line
• The Displaced Dusty ISM of NGC 3077: Tidal Stripping in the M 81 Triplet
• Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The C--D Band Strengths of Mono-Deuterated Species
• More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
• A Direct Measurement of the Dust Extinction Curve in an Intermediate-Redshift Galaxy
• Characterizing Ultraviolet and Infrared Observational Properties for Galaxies. II. Features of Attenuation Law
• Ultracompact H II Regions with Extended Emission: The Complete View
• The dust properties and physical conditions of the interstellar medium in the LMC massive star forming complex N11
• Variation of the Nebular Dust Attenuation Curve with the Properties of Local Star-forming Galaxies
• ISM conditions in z~0.2 Lyman-Break Analogs
• 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
• Far-infrared extinction mapping of infrared dark clouds
• Deuterated Polycyclic Aromatic Hydrocarbons in the Interstellar Medium: The C--D Band Strengths of Multi-Deuterated Species
• Far-infrared dust properties in the Galaxy and the Magellanic Clouds
• Interstellar Extinction and Elemental Abundances: Individual Sight Lines
• DFT study of five-membered ring PAHs
• ISO observations of 3 - 200 micron emission by three dust populations in an isolated local translucent cloud
• Dust Extinction Law in Nearby Star-Resolved Galaxies. I. M31 Traced by Supergiants
• Dust in AGB wind-ISM interaction regions
• Variations between Dust and Gas in the Diffuse Interstellar Medium. 3. Changes in Dust Properties
• Modelling the spectral energy distribution of galaxies: introducing the artificial neural network
• High contrast and resolution near infrared photometry of the core of R136
• Effects of turbulent dust grain motion to interstellar chemistry
• Dust accretion and destruction in galaxy groups and clusters
• The Physical Drivers of the Luminosity-Weighted Dust Temperatures in High-Redshift Galaxies
• Chemical modelling of dust-gas chemistry within AGB outflows -- II. Effect of the dust-grain size distribution
• Molecular Gas Kinematics and Star Formation Properties of the Strongly-Lensed Quasar Host Galaxy RXS J1131-1231
• Modeling and predicting the shape of the far-infrared to submillimeter emission in ultra-compact HII regions and cold clumps
• Runaway stars masquerading as star formation in galactic outskirts
• Evolution of PAHs in protoplanetary disks
• Revisiting the lifetime estimate of large presolar grains in the interstellar medium
• Cospatial Star Formation and Supermassive Black Hole Growth in $z\sim 3$ Galaxies: Evidence for In-situ Co-evolution
• Dust Extinction Law in Nearby Star-Resolved Galaxies. II. M33 Traced by Supergiants
• Si isotope homogeneity of the solar nebula
• Interstellar dust properties of M51 from AKARI mid-infrared images
• Interstellar Silicate Dust in the z=0.685 Absorber Toward TXS 0218+357
• Systematic errors in dust mass determinations: Insights from laboratory opacity measurements
• Constrained simulations of the Antennae Galaxies: Comparison with Herschel-PACS observations
• The role of grain size in AGN torus dust models
• 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
• On the stability of non-isothermal Bonnor-Ebert spheres. II. The effect of gas temperature on the stability
• Herschel/PACS Observations of the Host Galaxy of GRB 031203
• Molecular Hydrogen Formation During Dense Interstellar Cloud Collapse
• The Spitzer View of Low-Metallicity Star Formation: II. Mrk 996, a Blue Compact Dwarf Galaxy with an Extremely Dense Nucleus
• Modelling Herschel observations of infrared-dark clouds in the Hi-GAL survey
• Spectropolarimetric Constraints on the Nature of Interstellar Grains
• Observations of PAHs in the atmospheres of discs and exoplanets
• Photon-Dominated Region Modeling of the [C I],[C II], and CO Line Emission from a Boundary in the Taurus Molecular Cloud
• Classification Study of WISE Infrared Sources: Identification of Candidate Asymptotic Giant Branch Stars
• A resolved and asymmetric ring of PAHs within the young circumstellar disk of IRS 48
• On the Diagnostic Power of FIR/Sub-mm SED Fitting in Massive Galactic Molecular Clumps
• Polycyclic Aromatic Hydrocarbons in Exoplanet Atmospheres I. Thermochemical Equilibrium Models
• First MATISSE L-band observations of HD 179218. Is the inner 10 au region rich in carbon dust particles?
• The Long-Term Secular Mass Accretion Rate of the Recurrent Nova T Pyxidis
• SPAMCART: a code for smoothed particle Monte Carlo radiative transfer
• The protoplanetary disc around HD 169142: circumstellar or circumbinary?
• ExoVista: A Suite of Planetary System Models for Exoplanet Studies
• Temperature Variations of the Cold Dust in the Triangulum Galaxy M33
• Continuum Observations of M51 and M83 at 1.1 mm with AzTEC
• Properties of dust and PAHs in the hot plasma of the elliptical galaxy NGC4125 revealed with AKARI and Spitzer
• Observations of 6 - 200 μm emission of the Ophiuchus cloud LDN 1688
• JWST observations of the Horsehead photon-dominated region I. First results from multi-band near- and mid-infrared imaging
• Implications of Grain Size Distribution and Composition for the Correlation Between Dust Extinction and Emissivity
• Structure Generation by Irradiation: What can GLIMPSE teach us about the ISM structure?
• The impact of accretion heating and thermal conduction on the dead zone of protoplanetary disks
• The scattering and extinction properties of nanodiamonds
• The failure of testing for cosmic opacity via the distance-duality relation
• Fully Sampled Maps of Ices and Silicates in Front of Cepheus A East with Spitzer
• Characteristics of mid-infrared PAH emission from star-forming galaxies selected at 250 μm in the North Ecliptic Pole (NEP) field
• Observations of Free-Free and Anomalous Microwave Emission from LDN 1622 with the 100 m Green Bank Telescope
• Effects of dust abundance on the far-infrared colours of blue compact dwarf galaxies
• Circumgalactic Ly$\alpha$ emission around submillimeter-bright galaxies with different quasar contributions
• Resonant infrared irradiation of CO and CH3OH interstellar ices
• A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
• Nanodust in the Interstellar Medium in Comparison to the Solar System
• Are the Formation and Abundances of Metal-Poor Stars the Result of Dust Dynamics?
• Extraplanar gas in Edge-on Galaxies traced by SOFIA observations of [C II]
• Is the mm/submm dust polarization a robust tracer of the magnetic field topology in protostellar envelopes? A model exploration
• Scattered H-alpha emission from a large translucent cloud G294-24
• On Carbon Nanotubes in the Interstellar Medium
• Kathryns Wheel: A spectacular galaxy collision discovered in the Galactic neighbourhood
• Feasibility of detecting shadows in disks induced by infall
• Spectral energy distributions of dust and PAHs based on the evolution of grain size distribution in galaxies
• Mid-infrared imaging and modelling of the dust shell around post-AGB star HD 187885 (IRAS 19500-1709)
• Impact of Dust on Spectral Distortion Measurements of the Cosmic Microwave Background
• Molecular gas budget and characterization of intermediate-mass star-forming galaxies at $z\approx 2-3$
• A panchromatic view of star cluster formation in a simulated dwarf galaxy starburst
• The physical state of selected cold clumps
• Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
• The HI supershell GS 118+01-44 and its role in the interstellar medium
• Modeling IR Spectral Energy Distributions: A Pilot Study of Starburst Parameters and Silicate Absorption Curves for Some GOALS Galaxies
• Limits on Intergalactic Dust During Reionization
• Infrared Spectral Energy Distribution of Galaxies in the AKARI All Sky Survey: Correlations with Galaxy Properties, and Their Physical Origin
• Near- to mid-Infrared Observations of Galaxy Mergers: NGC2782 and NGC7727
• Radiative transfer of ionizing radiation through gas and dust: grain charging in star forming regions
• Evolution of dust grain size distribution and grain porosity in galaxies
• Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
• Linear dust polarization during the embedded phase of protostar formation
• The edge-on disk Tau042021: icy grains at high altitudes and a wind containing astronomical PAHs
• Dense Gas and Star Formation in Nearby Infrared Bright Galaxies: APEX survey of HCN and HCO+ J=2-1
• Restructuring and destruction of hydrocarbon dust in the interstellar medium
• The complex infrared dust continuum emission of NGC1068: ground-based N- and Q-band spectroscopy and new radiative transfer models
• Dust Models for the Extinction of Type IIn Supernova SN 2010jl
• Dissecting the central regions of OH 231.8 + 4.2 with ALMA: a salty rotating disk at the base of a young bipolar outflow
• Extinction calculations of multi-sphere polycrystalline graphitic clusters - A comparison with the 2175 AA peak and between a rigorous solution and discrete-dipole approximations
• Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER
• 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
• ALMA Lensing Cluster Survey: A spectral stacking analysis of [CII] in lensed $z\sim 6$ galaxies
• Correlation between UV resilience and wavelength of narrow DIBs
• A new galaxy spectral energy distribution model consistent with the evolution of dust
• Sunscreen: Photometric Signatures of Galaxies Partially Cloaked in Dyson Spheres
• Dust Extinction towards the Type Ia Supernova 2012cu in NGC 4772
• Missing dust signature in the cosmic microwave background
• 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
• Evidence of Extended Dust and Feedback around z$\approx$1 Quiescent Galaxies via Millimeter Observations
• LABOCA and MAMBO-2 imaging of the dust ring of the Sombrero galaxy (NGC 4594)
• The 2175 Angstrom Interstellar Extinction Bump: Is the Wavelength Variable?
• The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities
• Optical and Infrared Imaging and Spectroscopy of the Multiple-Shell Planetary Nebula NGC 6369
• Grain Physics and Rosseland Mean Opacities
• Radiative Transfer Modeling of An SN 1987A Light Echo$-$AT2019xis
• Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova
• Dust emission at 8-mic and 24-mic as Diagnostics of HII Region Radiative Transfer
• Effects of rotational disruption on the evolution of grain size distribution in galaxies
• The role of molecular gas in the nuclear regions of IRAS 00183-7111. ALMA and X-ray investigations of an ultraluminous infrared galaxy
• Enhanced dust emissivity power-law index along the western H$\alpha$ filament of NGC 1569
• Gathering dust: A galaxy-wide study of dust emission from cloud complexes in NGC 300
• Extinction Laws toward Stellar Sources within a Dusty Circimstellar Medium and Implications for Type Ia Supernovae
• Spectroscopic infrared extinction mapping as a probe of grain growth in IRDCs
• Modelling galaxy spectra in presence of interstellar dust-III. From nearby galaxies to the distant Universe
• Dark Dust III: The high-quality single-cloud reddening curve sample. Scrutinizing extinction curves in the Milky Way
• Observational signatures of the dust size evolution in isolated galaxy simulations
• SMART: spectral energy distributions Markov chain analysis with radiative transfer models
• Dust-Evacuated Zones Near Massive Stars: Consequences of Dust Dynamics on Star-forming Regions
• ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion
• Spinning Dust Emission from Wobbling Grains: Important Physical Effects and Implications
• Dust Emission from Evolved and Unevolved HII Regions in the Large Magellanic Cloud
• Importance of far-infrared mapping in a spiral galaxy: AKARI observation of M81
• Thermal emission from the amorphous dust: An alternative possibility of the origin of the anomalous microwave emission
• Ultraviolet extinction properties of the 30 Dor Nebula and interpreting observations of starburst clusters
• The incidence of mid-infrared excesses in G and K giants
• Spatially resolved dust emission of extremely metal poor galaxies
• A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
• Spatial distribution of the aromatic and aliphatic carbonaceous nano-grain features in the protoplanetary disk around HD 100546
• UV-FIR SED modeling of AGN in IR-luminous galaxies up to z~2.5: Understanding the effects of torus models
• Spatially resolving polycyclic aromatic hydrocarbons in Herbig Ae disks with VISIR-NEAR at the VLT
• Observing the Earliest Stages of Star Formation in Galaxies: 8 micron Cores in Three Edge-on Disks
• The Physical Characteristics of Interstellar Medium in NGC 3665 with Herschel Observations
• A probable Keplerian disk feeding an optically revealed massive young star
• Searching for a cometary belt around Trappist-1 with ALMA
• 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
• Dust in the Local Group
• Signature of outflows in strong MgII absorbers in quasar sightlines
• Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization
• Carbon 'fluffy' aggregates produced by helium - hydrocarbon high pressure plasmas as analogs to interstellar dust
• A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
• Modelling Grain Rotational Disruption by Radiative Torques and Extinction of Active Galactic Nuclei
• Cosmic Biology in Perspective
• Effect of surface H${}_2$ on molecular hydrogen formation on interstellar grains
• Mid-IR FORCAST/SOFIA Observations of M82
• What causes the ultraviolet extinction bump at the cosmic dawn?
• Five new hot-Jupiter transits investigated with Swift-UVOT
• A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements
• 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
• 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
• Detectability of Polycyclic Aromatic Hydrocarbons in the Atmosphere of WASP-6 b with JWST NIRSpec PRISM
• Search for signatures of dust in the Pluto-Charon system using Herschel/PACS observations
• On the Absorption Properties of Metallic Needles
• A deep-learning approach to the 3D reconstruction of dust density and temperature in star-forming regions
• Dust Properties of Clumpy Disc Galaxies at z~1.3 with Herschel-SPIRE
• 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
• Revisiting the Local Interstellar Radiation Field using Gaia DR3
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• Dust Mass Associated with the Supernova Remnant IC 443 when Emission Meets Extinction
• The Cosmic-Ray Induced Sputtering Process On Icy Grains
• [CII] emission properties of the massive star-forming region RCW36 in a filamentary molecular cloud
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Impact of dust diffusion on the rim shape of protoplanetary disks
• Recent Results of Solid-State Spectroscopy
• Comparing Infrared Star-Formation Rate Indicators with Optically-Derived Quantities
• Detection of an ultra-bright submillimeter galaxy behind the Small Magellanic Cloud
• Synthetic observations of protostellar multiple systems
• New Mid-Infrared Imaging Constraints on Companions and Protoplanetary Disks around six Young Stars
• The Wyoming Survey for H-alpha. III. A Multi-wavelength Look at Attenuation by Dust in Galaxies out to z~0.4
• Fast radiative transfer of dust reprocessing in semi-analytic models with artificial neural networks
• Processing of hydrocarbon dust in star-forming galaxies revealed with AKARI
• Mid-infrared extinction toward the Galactic center
• UV/Optical/IR Color Sequences Along the Tidal Ring/Arm of Arp 107
• Global Spectral Energy Distributions of the Large Magellanic Cloud with Interstellar Dust
• The impact of cosmic ray feedback during the epoch of reionisation
• The Radial Profile of Dust Grain Size in the Protoplanetary Disk of DS Tau
• On planet formation around supermassive black holes and the grain disruption barriers by radiative torques
• Characterizing elusive, faint dusty star-forming galaxies: a lensed, optically undetected ALMA galaxy at z~3.3
• Molecules with ALMA at Planet-forming Scales (MAPS) XVII: Determining the 2D Thermal Structure of the HD 163296 Disk
• A Massive Gas Outflow Outside the Line-of-Sight: Imaging Polarimetry of the Blue Excess Hot Dust Obscured Galaxy W0204-0506
• ALMA Lensing Cluster Survey: Dust mass measurements as a function of redshift, stellar-mass and star formation rate, from z=1 to z=5
• Estimation of high-resolution dust column density maps: Empirical model fits
• 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
• SPHEREx: Aromatics, Aliphatics and PAH Size across the Iris Nebula
• GATOS XI : Excess dust heating in the Narrow Line Regions of nearby AGN revealed with JWST/MIRI
• Modelling the SEDs of spiral galaxies
• A simple model of dust extinction in gamma-ray burst host galaxies
• NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
• Magnetism of Fullerene C60 Compared with Graphene Molecule by DFT Calculation, Laboratory Experiment and Astronomical Observation
• The Binding Energies of Atoms on Amorphous Silicate Dust: A Computational Study
• MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
• Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
• Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs
• 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
• Effects of grain temperature distribution on organic protostellar envelope chemistry
• Interstellar Grains: Effect of Inclusions on Extinction
• Outflows from starburst galaxies with various driving mechanisms and their X-ray properties
• The Large Magellanic Cloud: A power spectral analysis of Spitzer images
• A systematic study on the properties of aromatic and aliphatic hydrocarbon dust in active galactic nuclei with AKARI near-infrared spectroscopy
• Polycyclic aromatic hydrocarbon (PAH) abundances in the disk around T Chamaeleontis (T Cha): PAH sizes, ionization fraction, and mass during JWST observations
• Studying the spectral properties of Active Galactic Nuclei in the JWST era
• Analytic formulas for frequency and size dependence of absorption and scattering efficiencies of astronomical polycyclic aromatic hydrocarbons
• Optical constants of Ih, Ic, and amorphous H${}_2$O ices in the THz and IR ranges
• An Improved Pair Method to Probe the Dust Extinction Law
• The role of young and evolved stars in the heating of dust in local galaxies
• Void defect induced magnetism and structure change of carbon material-3, Polycyclic aromatic hydrocarbon
• Exploring the 100 au Scale Structure of the Protobinary System NGC 2264 CMM3 with ALMA
• MINDS survey of silicates in T Tauri disks: Correlation between dust and gas
• Do We Have Sufficient Knowledge of the Galactic Foreground Emission in Cosmic Microwave Background Science?
• Better Alternative to "Astronomical Silicate": Laboratory-Based Optical Functions of Chondritic/Solar Abundance Glass With Application to HD161796
• Modeling Long-Wavelength Amorphous Dust Emission Based on the Physically Motivated Soft-Potential Model
• Constraining the Metallicities of Damped Ly$\alpha$ Systems Using Extinction Curves
• A Detailed Analysis of Intermediate-scale Structure in Optical Extinction Curves: Expanded Census and Two-family Classification
• Dense Star-forming Gas and Dust in the Magellanic Clouds
• A Semi-Empirical Model of the Infrared Emission from Galaxies
• What is the amount of baryonic dark matter in galaxies?