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Publications of the Astronomical Society of Japan, ISSN 0004-6264, 05/2018, Volume 70, Issue SP2, pp. S411 - S4118
Abstract We carried out new CO (J = 1–0, 2–1, and 3–2) observations with NANTEN2 and ASTE in the region of the twin Galactic mini-starbursts NGC 6334 and NGC... 
ISM: individual objects (NGC 6334, NGC 6357) | stars: formation | ISM: clouds | COMPLEX | PHASE | ASTRONOMY & ASTROPHYSICS | WESTERLUND 2 | STAR-FORMATION | GAS | CLUSTER | Physics - Astrophysics of Galaxies
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 11/2019, Volume 886, Issue 1, p. 14
We present ALMA observations of CO isotopes and 1.3 mm continuum emission toward the N159E-Papillon Nebula in the Large Magellanic Cloud (LMC). The spatial... 
stars: formation | stars: protostars | ASTRONOMY & ASTROPHYSICS | ISM: kinematics and dynamics | GAS | STELLAR POPULATIONS | ISM: clouds | ISM: individual (N159E) | J=3-2 | 2ND SURVEY | Physics - Astrophysics of Galaxies
Journal Article
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, 06/2018, Volume 859, Issue 2, p. 86
This paper reports a re-analysis of archival ALMA data of the high velocity (-width) compact cloud (HVCC) CO-0.40-0.22, which has recently been hypothesized to... 
ISM: clouds | Galaxy: center | ISM: abundances | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2019, Volume 485, Issue 4, pp. 4509 - 4528
We perform ideal magnetohydrodynamics high-resolution adaptive mesh refinement simulations with driven turbulence and self-gravity and find that long... 
ISM:Evolution | ISM: Magnetic fields | ISM: Kinematics and dynamics | turbulence | ISM: Clouds | methods: Numerical | HELICAL FIELDS | GRAVITATIONAL-INSTABILITY | ISM: evolution | ASTRONOMY & ASTROPHYSICS | ISM: kinematics and dynamics | GAS | ISM: clouds | SIMULATIONS | methods: numerical | FRAGMENTATION | ISM: magnetic fields
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
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 05/2018, Volume 476, Issue 2, pp. 2209 - 2219
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2019, Volume 484, Issue 4, pp. 5734 - 5754
The evolution of molecular clouds in galactic centres is thought to differ from that in galactic discs due to a significant influence of the external... 
Galaxy: Centre | ISM: Evolution | ISM: Kinematics and dynamics | Stars: Formation | ISM: Clouds | Galaxies: ISM | ROTATION | ISM: evolution | STARBURSTS | ISM: kinematics and dynamics | ENVIRONMENT | STAR-FORMATION | COLLISION | stars: formation | PLANE SURVEY HOPS | Galaxy: centre | galaxies: ISM | ASTRONOMY & ASTROPHYSICS | GAS | ISM: clouds | CONTINUUM | GALAXIES | MILKY-WAY
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 05/2018, Volume 70, Issue SP2, pp. S461 - S4613
Abstract We carried out a molecular-line study toward the three Spitzer bubbles S116, S117, and S118, which show active formation of high-mass stars. We found... 
stars: formation | ISM: clouds | ISM: individual objects (S116, S117, S118) | RADIO IMAGING SURVEY | SUMSS | ASTRONOMY & ASTROPHYSICS | SOUTHERN SKY | RCW 120 | BORDERS | PARAMETERS | O-STARS | MASSIVE-STAR-FORMATION
Journal Article