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20102014
most citedMolecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

164 citations · 440 across the 7 of their papers we have counts for

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5 papers · 1 filter

astro-ph.GA2014★ 11 cited

The jet and arc molecular clouds toward Westerlund 2, RCW 49, and HESS J1023-575; 12CO and 13CO (J=2-1 and J=1-0) observations with NANTEN2 and Mopra Telescope

N. Furukawa, A. Ohama, T. Fukuda +20

We have made new CO observations of two molecular clouds, which we call "jet" and "arc" clouds, toward the stellar cluster Westerlund 2 and the TeV gamma-ray source HESS J1023-575.…

astro-ph.GA2013★ 164 cited

Molecular Clouds Toward the Super Star Cluster NGC3603; Possible Evidence for a Cloud-Cloud Collision in Triggering the Cluster Formation

Yasuo Fukui, Akio Ohama, Naoki Hanaoka +17

We present new large field observations of molecular clouds with NANTEN2 toward the super star cluster NGC3603 in the transitions 12CO(J=2-1, J=1-0) and 13CO(J=2-1, J=1-0). We sugg…

astro-ph.GA2010★ 38 cited

Dense Clumps in Giant Molecular Clouds in the Large Magellanic Cloud: Density and Temperature Derived from CO() Observations

Tetsuhiro Minamidani, Takanori Tanaka, Yoji Mizuno +17

In order to precisely determine temperature and density of molecular gas in the Large Magellanic Cloud, we made observations of optically thin CO() transition by usin…

astro-ph.GA2010★ 15 cited

High Excitation Molecular Gas in the Galactic Center Loops; 12CO(J =2-1 and J =3-2) Observations

Natsuko Kudo, Kazufumi Torii, Mami Machida +18

We have carried out 12CO(J =2-1) and 12CO(J =3-2) observations at spatial resolutions of 1.0-3.8 pc toward the entirety of loops 1 and 2 and part of loop 3 in the Galactic center w…

astro-ph.GA2010★ 80 cited

Star Forming Dense Cloud Cores in the TeV γ-ray SNR RX J1713.7-3946

H. Sano, J. Sato, H. Horachi +23

RX J1713.7-3946 is one of the TeV γ-ray supernova remnants (SNRs) emitting synchrotron X rays. The SNR is associated with molecular gas located at ~1 kpc. We made new molecular obs…