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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
Annual Review of Astronomy and Astrophysics, ISSN 0066-4146, 9/2012, Volume 50, Issue 1, pp. 29 - 63
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 446, Issue 4, pp. 3608 - 3620
We investigate cloud-cloud collisions and giant molecular cloud evolution in hydrodynamic simulations of isolated galaxies. The simulations include heating and... 
ISM: clouds | ISM: evolution | Stars: formation | Galaxies: ISM | VELOCITY DISPERSION | STELLAR FEEDBACK | SMOOTHED PARTICLE HYDRODYNAMICS | CLUSTER FORMATION | INTERSTELLAR CLOUDS | stars: formation | DISK GALAXIES | SPIRAL STRUCTURE | GIANT MOLECULAR CLOUDS | STAR-FORMATION RATES | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | GALACTIC-CENTER
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
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 465, Issue 3, pp. 3483 - 3494
In an earlier paper, we used smoothed particle hydrodynamics (SPH) simulations to explore star formation triggered by head-on collisions between... 
Stars: kinematics and dynamics | CORES | EVOLUTION | MOLECULAR CLOUDS | COLLAPSE | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | GAS | stars: kinematics and dynamics | SPH | SIMULATIONS | Fluid mechanics | Clouds | Star & galaxy formation | Velocity | Astronomy
Journal Article