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Astrophysical Journal, ISSN 0004-637X, 03/2016, Volume 820, Issue 1, pp. 26 - 26
We present distributions of two molecular clouds having velocities of 2 and 14 km s super(-1) toward RCW 38, the youngest super star cluster in the Milky Way,... 
stars: formation | ISM: clouds | ISM: molecules | ISM: kinematics and dynamics | O stars | Clouds | Molecular clouds | Milky Way Galaxy | Clusters | Emission | Formations | Star clusters | STAR CLUSTERS | VELOCITY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | CARBON 13 | STAR EVOLUTION | CLOUDS | STARS | MILKY WAY | CARBON MONOXIDE | COLLISIONS | COSMIC DUST | MOLECULES
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2017, Volume 837, Issue 1, p. 44
To probe star formation (SF) processes, we present results of an analysis of the molecular cloud G35.20-0.74 (hereafter MCG35.2) using multi-frequency... 
ISM: clouds | extinction | H II regions | dust | FIELD | INFRARED SURVEY | ISOLATING SIGNATURES | dust, extinction | GALACTIC PLANE | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | REGIONS | PROTOSTARS | SPITZER OBSERVATIONS | CLUSTER | POLARIZATION | Physics - Solar and Stellar Astrophysics
Journal Article
Bulletin of the American Meteorological Society, ISSN 0003-0007, 5/2016, Volume 97, Issue 5, pp. 787 - 802
Clouds over the ocean, particularly throughout the tropics, are poorly understood and drive much of the uncertainty in model-based projections of climate... 
ARTICLES | SCHEME | DUST | PROFILES | TRADE-WIND CUMULI | RADAR | PACIFIC | OCEAN | MASS | SHALLOW CUMULUS | METEOROLOGY & ATMOSPHERIC SCIENCES | Weather | Measurement | Hydrology | Global temperature changes | Investigations | Radiation | Studies | Climate change | Wind | Observatories | Clouds | General circulation models | Science | Remote sensing
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2017, Volume 603, p. A90
Journal Article
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 9/2012, Volume 50, Issue 1, pp. 29 - 63
Journal Article
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
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