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astronomy & astrophysics (282) 282
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Astrophysical Journal, ISSN 0004-637X, 07/2018, Volume 861, Issue 1, p. 19
In the direction of l = 17 degrees.6-19 degrees, the star-forming sites Sh 2-53 and IRAS 18223-1243 are prominently observed, and seem to be physically... 
stars: formation | ISM: clouds | dust, extinction | H II regions | ISM: individual object (IRAS 18223-1243) | MOLECULAR CLOUDS | MASS PROTOSTELLAR CANDIDATES | ISOLATING SIGNATURES | LIFETIMES | CLUSTERS | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | INFRARED DARK CLOUDS | CONTINUUM | EMISSION | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 06/2015, Volume 578, p. A29
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 08/2004, Volume 422, Issue 2, pp. 573 - 585
We present a detailed analysis of the diagnostic properties of methanol, (CH3OH), in dense molecular clouds, made possible by the availability of new... 
Molecular processes | ISM: molecules | ISM: clouds | CORES | MULTITRANSITION | POPULATION | AMMONIA | ISM : molecules | INFRARED-DARK CLOUDS | ROTATIONAL-EXCITATION | ISM : clouds | ASTRONOMY & ASTROPHYSICS | THERMOMETER | molecular processes | CHEMISTRY | TRANSITIONS | EXCITED TORSIONAL STATES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 4, pp. 3667 - 3683
We study the properties of giant molecular clouds (GMCs) from a smoothed particle hydrodynamics simulation of a portion of a spiral galaxy, modelled at high... 
ISM: Structure | ISM: Clouds | Galaxies: ISM | Galaxies: Spiral | PHYSICAL-PROPERTIES | STAR-FORMING GALAXIES | INTERSTELLAR-MEDIUM | ISM: structure | GALACTIC PLANE SURVEY | SCALING RELATIONS | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | RING SURVEY | ISM: clouds | INFRARED DARK CLOUD | MILKY-WAY | galaxies: spiral | NEARBY SPIRAL GALAXIES | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A89
The central molecular zone (CMZ; inner similar to 200 pc) of the Milky Way is a star formation (SF) environment with very extreme physical properties.... 
Stars: formation | ISM: clouds | Methods: data analysis | H II REGION | methods: data analysis | MAGNETIC-FIELDS | SGR A-ASTERISK | SAGITTARIUS-D | INFRARED-DARK CLOUDS | H2O MASERS | CONTINUUM EMISSION | YOUNG STELLAR OBJECTS | stars: formation | CENTER DUST RIDGE | ASTRONOMY & ASTROPHYSICS | MILKY-WAY | Physics - Astrophysics of Galaxies
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 06/2010, Volume 716, Issue 1, pp. 433 - 445
Journal Article
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 03/2013, Volume 765, Issue 2, pp. L35 - 6
Journal Article