activity
20072011
most citedThe Second Survey of the Molecular Clouds in the Large Magellanic Cloud by NANTEN. II. Star Formation

299 citations · 1.3k across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2011★ 266 cited

The Magellanic Mopra Assessment (MAGMA). I. The Molecular Cloud Population of the Large Magellanic Cloud

Tony Wong, Annie Hughes, Jürgen Ott +15

We present the properties of an extensive sample of molecular clouds in the Large Magellanic Cloud (LMC) mapped at 11 pc resolution in the CO(1-0) line. We identify clouds as regio…

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.CO2010★ 126 cited

Physical Properties of Giant Molecular Clouds in the Large Magellanic Cloud

A. Hughes, T. Wong, J. Ott +14

The Magellanic Mopra Assessment (MAGMA) is a high angular resolution CO mapping survey of giant molecular clouds (GMCs) in the Large and Small Magellanic Clouds using the Mopra Tel…

astro-ph.GA2010★ 44 cited

Characterizing the Low-Mass Molecular Component in the Northern Small Magellanic Cloud

E. Muller, J. Ott, A. Hughes +8

We present here the first results from a high-resolution survey of the 12CO(J=1-0) emission across the northern part of the poorly-enriched Small Magellanic Cloud, made with the AT…

astro-ph.CO2009★ 40 cited

Warm and Dense Molecular Gas in the N159 Region: 12CO J=4-3 and 13CO J=3-2 Observations with NANTEN2 and ASTE

Yoji Mizuno, Akiko Kawamura, Toshikazu Onishi +29

New 12CO J=4-3 and 13CO J=3-2 observations of the N159 region in the Large Magellanic Cloud have been made. The 12CO J=4-3 distribution is separated into three clumps. These new me…

astro-ph.GA2009★ 85 cited

Molecular and Atomic Gas in the Large Magellanic Cloud II. Three-dimensional Correlation between CO and HI

Y. Fukui, A. Kawamura, T. Wong +10

We compare the CO J =(1-0) and HI emission in the Large Magellanic Cloud (LMC) in three dimensions, i.e. including a velocity axis in addition to the two spatial axes, with the aim…