activity
20022026
most citedSpitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

718 citations · 4.4k across the 62 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.GA2016★ 107 cited

Triggered O star formation in M20 via cloud-cloud collision: Comparisons between high-resolution CO observations and simulations

Kazufumi Torii, Yusuke Hattori, Keisuke Hasegawa +9

High-mass star formation is one of the top-priority issues in astrophysics. Recent observational studies are revealing that cloud-cloud collisions may play a role in high-mass star…

astro-ph.GA2016★ 24 cited

An analysis of star formation with Herschel in the Hi-GAL Survey. II. The tips of the Galactic bar

M. Veneziani, E. Schisano, D. Elia +20

We present the physical and evolutionary properties of prestellar and protostellar clumps in the Herschel Infrared GALactic plane survey (Hi-GAL) in two large areas centered in the…

astro-ph.GA2016★ 51 cited

Kinematic Structure of Molecular Gas around High-mass Star YSO, Papillon Nebula, in N159 East in the Large Magellanic Cloud

Kazuya Saigo, Toshikazu Onishi, Omnarayani Nayak +20

We present the ALMA Band 3 and Band 6 results of 12CO(2-1), 13$CO(2-1), H30alpha recombination line, free-free emission around 98 GHz, and the dust thermal emission around 230 GHz…

astro-ph.GA2016★ 8 cited

Detection of a turbulent gas component associated with a starless core with subthermal turbulence in the Orion A cloud

Satoshi Ohashi, Ken'ichi Tatematsu, Patricio Sanhueza +4

We report the detection of a wing component in NH emission toward the starless core TUKH122 with subthermal turbulence in the Orion A cloud. This NH core is suggested to be…

astro-ph.GA2016★ 46 cited

Angular Momentum of the N2H+ Cores in the Orion A Cloud

Ken'ichi Tatematsu, Satoshi Ohashi, Patricio Sanhueza +3

We have analyzed the angular momentum of the molecular cloud cores in the Orion A giant molecular cloud observed in the N2H+ J = 1-0 line with the Nobeyama 45 m radio telescope. We…