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Proceedings of the National Academy of Sciences of the United States of America, ISSN 0027-8424, 6/2012, Volume 109, Issue 26, pp. 10233 - 10238
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2013, Volume 553, pp. A119 - 18
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2014, Volume 562, pp. A83 - np
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2012, Volume 542, p. A77
We analyze the physical parameters of interstellar filaments that we describe by an idealized model of isothermal self-gravitating infinite cylinder in... 
Infrared: ISM | ISM: clouds | Submillimeter: ISM | Stars: formation | ISM: structure | FIELDS | GOULD BELT | MOLECULAR CLOUDS | STAR-FORMATION | infrared: ISM | DEPLETION | OBJECTS | stars: formation | AQUILA | submillimeter: ISM | PERSEUS | ASTRONOMY & ASTROPHYSICS | DENSE CORES | EQUILIBRIUM | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, Supplement Series, ISSN 0067-0049, 06/2016, Volume 224, Issue 2, pp. 42 - 42
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 04/2007, Volume 466, Issue 1, pp. 215 - 228
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2019, Volume 485, Issue 1, pp. 1220 - 1247
We investigate the equilibrium charge distribution of dust grains in the interstellar medium (ISM). Our treatment accounts for collisional charging by... 
ADAPTIVE MESH REFINEMENT | MAGNETOHYDRODYNAMIC SHOCK-WAVES | STAR-FORMATION | RADIATION-FIELD | PHOTOELECTRIC-EMISSION | DESTRUCTION | dust, extinction | cosmic rays | MOLECULAR CLOUD EVOLUTION | ASTRONOMY & ASTROPHYSICS | GRAIN-GRAIN COLLISIONS | ISM: clouds | DENSE CLOUDS | IONIZATION
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2016, Volume 457, Issue 1, pp. 375 - 388
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 09/2006, Volume 648, Issue 1 I, pp. 461 - 471
We present large velocity gradient (LVG) and nonlocal radiative transfer calculations involving the rotational and hyperfine structure of the spectrum of N2H+,... 
Line: formation | Molecular processes | ISM: molecules | ISM: abundances | ISM: clouds | Radiative transfer | Line: profiles | radiative transfer | ISM : abundances | ISM : molecules | line : profiles | HN-2 | line : formation | ROTATIONAL-EXCITATION | DARK CLOUDS | ISM : clouds | HCO | ASTRONOMY & ASTROPHYSICS | DENSE CORES | molecular processes
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 05/2015, Volume 577, p. L5
We conducted radioastronomical observations of 9 dark clouds with the IRAM 30 m telescope. We present the first identification in space of the ketenyl radical... 
Line: identification | Astrochemistry | ISM: clouds | ISM: molecules | Radio lines: ISM | ANIONS | ORGANIC-MOLECULES | COMPLEX | COMBUSTION | ICES | GAS-PHASE CHEMISTRY | OXYGEN | radio lines: ISM | SPECTROSCOPY | ASTRONOMY & ASTROPHYSICS | DENSE CORES | COLD DARK CLOUDS | line: identification | astrochemistry | Propylene | Clouds | Counterbalances | Density | Ketenes | Astronomy | Radicals | Acetaldehyde | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 08/2015, Volume 580, p. A136
Aims. We compare the performance of several dust models in reproducing the dust spectral energy distribution (SED) per unit extinction in the diffuse... 
Evolution | Dust, extinction | GRAINS | dust, extinction | HYDROCARBONS | MISSION | FIELD | ASTRONOMY & ASTROPHYSICS | SPITZER | evolution | DENSE MOLECULAR CLOUDS | EMISSION | EXTINCTION | POLARIZATION | Dust | Extinction | Optical properties | Emission | Mathematical models |