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Astrophysical Journal, ISSN 0004-637X, 02/2017, Volume 835, Issue 2
The process of atomic-to-molecular (H i-to-H2) gas conversion is fundamental for molecular-cloud formation and star formation. 21 cm observations of the... 
photondominated region (PDR) | ISM: clouds | ISM: individual objects (W43) | ISM: structure | galaxies: star formation | Cloud formation | Star formation | Star & galaxy formation | Radiation | Transition layers
Journal Article
Astronomy & Astrophysics, ISSN 1432-0746, 2018, Volume 616, pp. 1 - 22
Context. G24.78+0.08 is a well known high-mass star-forming region, where several molecular cores harboring OB young stellar objects are found inside a clump... 
Techniques: interferometric | ISM: jets and outflows | Radio continuum: ISM | ISM: molecules | Masers | radio continuum: ISM | CH3CN | VLA | masers | PARAMETERS | YOUNG STELLAR OBJECTS | MASER OBSERVATIONS | OUTFLOWS | ASTRONOMY & ASTROPHYSICS | GAS | techniques: interferometric
Journal Article
The Astrophysical Journal Letters, ISSN 1538-4357, 03/2008, Volume 675, Issue 1, pp. L33 - L36
Journal Article
Astrophysical Journal, ISSN 0004-637X, 10/2018, Volume 866, Issue 1, p. 61
Anderson et al. identified 76 candidate supernova remnants (SNRs) using data from the HI/OH/Recombination line survey of the Milky Way. The spectral index and... 
ISM: supernova remnants | polarization | ISM: H II regions | CATALOG | ASTRONOMY & ASTROPHYSICS | Supernova | Polarization | Supernova remnants | Candidates | H II regions | Pulsars | Milky Way Galaxy | Space telescopes | Linear polarization | Air pollution | Milky Way
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 01/2019, Volume 482, Issue 2, pp. 2681 - 2696
We have carried out the largest and most unbiased search for hypercompact (HC) H II regions. Our method combines four interferometric radio continuum surveys... 
MASSIVE STARS | submillimetre: ISM | ULTRACOMPACT HII-REGIONS | radio continuum: ISM | RESOLUTION | infrared: ISM | RECOMBINATION LINE | SPECTRAL INDEX | EVOLUTION | ASTRONOMY & ASTROPHYSICS | PROTOSTARS | RADIO | ACCRETION | STAR-FORMING REGION | ISM: H II regions
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2019, Volume 482, Issue 2, pp. 2681 - 2696
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 03/2018, Volume 611
Context. High-mass stars form in much richer environments than those associated with isolated low-mass stars, and once they reach a certain mass, produce... 
Comets | Accretion | Molecular gases | Bolometers | Stellar evolution | Velocity gradient | Velocity | Molecular chains | Massive stars | Emissions | Radio emission | Dynamic tests | Ionization | Morphology | Evolution | Star & galaxy formation | Deposition
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 0004-6361, 02/2020, Volume 634, p. A139
Molecular clouds form from the atomic phase of the interstellar medium. However, characterizing the transition between the atomic and the molecular... 
INTERSTELLAR-MEDIUM | COLUMN DENSITY | TRANSITION | stars: formation | DARK CLOUDS | RIEGEL | ISM: atoms | radio lines: ISM | TEMPERATURE | ISM: molecules | ASTRONOMY & ASTROPHYSICS | LINE | GAS | ISM: clouds | EXTINCTION | COLD HYDROGEN
Journal Article
Astronomy & Astrophysics, ISSN 0004-6361, 08/2015, Volume 580, p. A112
The aim of this paper is to study the atomic, molecular, and ionized emission of giant molecular clouds (GMC5) in the Milky Way, we initiated a large program... 
Molecular clouds | Pilots | Emission analysis | Continuums | Mathematical models | Density | Line of sight | Astronomy | Physics | Astrophysics
Journal Article