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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 01/2019, Volume 482, Issue 2, pp. 2555 - 2572
We revisit the evolution model of grain size distribution in a galaxy for the ultimate purpose of implementing it in hydrodynamical simulations. We simplify... 
STAR-FORMING CLOUDS | galaxies: evolution | INTERSTELLAR DUST | EXTINCTION CURVES | methods: numerical | ASYMPTOTIC GIANT BRANCH | SHOCKS | FRAGMENTATION | DUST FORMATION | COSMOLOGICAL SIMULATION | dust, extinction | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | COAGULATION | MILKY-WAY | galaxies: spiral | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2018, Volume 478, Issue 3, pp. 2851 - 2886
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2015, Volume 449, Issue 1, pp. 440 - 450
We consider dust drift under the influence of stellar radiation pressure during the pressure-driven expansion of an H II region using the chemo-dynamical model... 
Infrared: ISM | ISM: bubbles | Dust, extinction | TRAPEZIUM REGION | MOLECULAR CLOUDS | MAGNETIC-FIELDS | PHOTOELECTRIC SPECTROPHOTOMETRY | MAIN-SEQUENCE STARS | INTERSTELLAR DUST | infrared: ISM | TRIGGERED STAR-FORMATION | dust, extinction | ASTRONOMY & ASTROPHYSICS | FAR-INFRARED EMISSION | RCW 120 | HII-REGIONS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 2016, Volume 826, Issue 1, pp. 95 - 95
Journal Article
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 05/2011, Volume 732, Issue 2, p. 73
We investigate the formation of molecules during the chemical evolution of a cold dense interstellar cloud using a gas-grain numerical code in order to study... 
evolution | ISM: molecules | astrochemistry | ISM: abundances | DUST GRAINS | CORES | ICES | INTERSTELLAR CLOUDS | MODELS | ASTRONOMY & ASTROPHYSICS | REGIONS | MOLECULAR-HYDROGEN FORMATION | CHEMISTRY | COAGULATION | PHOTODESORPTION | DISTRIBUTION | PARTICLES | GRAIN SIZE | SIZE | ABUNDANCE | GRAIN GROWTH | MOLECULES | DENSITY | EVOLUTION | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | INTERSTELLAR GRAINS | CLOUDS | PHYSICAL PROPERTIES | MICROSTRUCTURE
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 1, pp. 1371 - 1383
In dense molecular clouds, interstellar grains are covered by mantles of iced molecules. The formation of the grain mantles has two important consequences: it... 
Astrochemistry | Galaxies: high-redshift | ISM: molecules | Galaxies: ISM | Dust, extinction | DEPLETION | SUPERNOVAE | ABUNDANCES | galaxies: high-redshift | PHASE | dust, extinction | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | MASS | CHEMISTRY | SURFACE | ATOMS | astrochemistry | GIANT BRANCH STARS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 447, Issue 3, pp. 2937 - 2950
Full calculations of the evolution of grain size distribution in galaxies are in general computationally heavy. In this paper, we propose a simple model of... 
Galaxies: evolution | dust, extinction | Methods: analytical | Galaxies: ISM | STAR-FORMING CLOUDS | DUST GRAINS | TO-GAS RATIO | galaxies: evolution | INTERSTELLAR DUST | EXTINCTION CURVES | FORMATION HISTORY | SILICON-CARBIDE | INFRARED-EMISSION | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | GROWTH | methods: analytical | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article