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Dust input from AGB stars in the Large Magellanic Cloud

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Astronomy & Astrophysics 555 A99 (2013)
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Proceedings of the International Astronomical Union 11 (S315) 191 (2015)
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HERschelKEY PROGRAM HERITAGE: A FAR-INFRARED SOURCE CATALOG FOR THE MAGELLANIC CLOUDS

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The Astronomical Journal 148 (6) 124 (2014)
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DUST AND GAS IN THE MAGELLANIC CLOUDS FROM THE HERITAGEHERSCHELKEY PROJECT. I. DUST PROPERTIES AND INSIGHTS INTO THE ORIGIN OF THE SUBMILLIMETER EXCESS EMISSION

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The Astrophysical Journal 797 (2) 85 (2014)
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Astronomy & Astrophysics 582 A28 (2015)
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Physical Properties of Molecular Clouds at 2 pc Resolution in the Low-metallicity Dwarf Galaxy NGC 6822 and the Milky Way

Andreas Schruba, Adam K. Leroy, J. M. Diederik Kruijssen, et al.
The Astrophysical Journal 835 (2) 278 (2017)
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Yasuo Fukui
Proceedings of the International Astronomical Union 8 (S292) 377 (2012)
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The dust properties and physical conditions of the interstellar medium in the LMC massive star-forming complex N11

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Monthly Notices of the Royal Astronomical Society 456 (2) 1767 (2016)
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The ISM of Low Metallicity Galaxies: The Herschel view

Suzanne C. Madden, Aurélie Rémy, Frédéric Galliano, et al.
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The evolution of the dust and gas content in galaxies

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Astronomy & Astrophysics 562 A30 (2014)
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Interstellar Extinction

G. A. Gontcharov
Astrophysics 59 (4) 548 (2016)
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A Statistical and Multi-wavelength Study of Star Formation in Galaxies

Corentin Schreiber
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Linking dust emission to fundamental properties in galaxies: the low-metallicity picture

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Astronomy & Astrophysics 582 A121 (2015)
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Millimeter dust emission compared with other mass estimates in N11 molecular clouds in the LMC

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Cool dust heating and temperature mixing in nearby star-forming galaxies

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The nature of the interstellar medium of the starburst low-metallicity galaxy Haro 11: a multi-phase model of the infrared emission

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The CO-to-H2Conversion Factor

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THE EVOLUTION OF DUST MASS IN THE EJECTA OF SN 1987A

Eli Dwek and Richard G. Arendt
The Astrophysical Journal 810 (1) 75 (2015)
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Variation in the dust emissivity index across M 33 withHerschelandSpitzer(HerM 33es)

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The Spatially Resolved Dust-to-metals Ratio in M101

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The Astrophysical Journal 865 (2) 117 (2018)
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Comprehensive comparison of models for spectral energy distributions from 0.1 μm to 1 mm of nearby star-forming galaxies

L. K. Hunt, I. De Looze, M. Boquien, et al.
Astronomy & Astrophysics 621 A51 (2019)
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On the diagnostic power of FIR/sub-mm SED fitting in massive galactic molecular clumps

Rebecca L Pitts, Peter J Barnes and Frank Varosi
Monthly Notices of the Royal Astronomical Society 484 (1) 305 (2019)
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Suppressed CO emission and high G/D ratios in z = 2 galaxies with sub-solar gas-phase metallicity

R T Coogan, M T Sargent, E Daddi, et al.
Monthly Notices of the Royal Astronomical Society 485 (2) 2092 (2019)
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PÉGASE.3: A code for modeling the UV-to-IR/submm spectral and chemical evolution of galaxies with dust

Michel Fioc and Brigitte Rocca-Volmerange
Astronomy & Astrophysics 623 A143 (2019)
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The Resolved Distributions of Dust Mass and Temperature in Local Group Galaxies

Dyas Utomo, I-Da Chiang, Adam K. Leroy, Karin M. Sandstrom and Jérémy Chastenet
The Astrophysical Journal 874 (2) 141 (2019)
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The JCMT Nearby Galaxies Legacy Survey — VIII. CO data and the LCO(3-2)-LFIR correlation in the SINGS sample

C. D. Wilson, B. E. Warren, F. P. Israel, et al.
Monthly Notices of the Royal Astronomical Society 424 (4) 3050 (2012)
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