3 citations · 4 across the 3 of their papers we have counts for
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Chandra Observation of the Starburst Galaxy NGC 2146
Tatsuya Inui, Hironori Matsumoto, Takeshi Go Tsuru +4
We present six monitoring observations of the starburst galaxy NGC 2146 using the Chandra X-ray Observatory. We have detected 67 point sources in the 8'.7 x 8'.7 field of view of t…
Starburst at the Expanding Molecular Superbubble in M82: Self-Induced Starburst at the Inner Edge of the Superbubble
Satoki Matsushita, Ryohei Kawabe, Kotaro Kohno +3
We present high spatial resolution (2.3"x1.9" or 43 pc x 36 pc at D = 3.9 Mpc) 100 GHz millimeter-wave continuum emission observations with the Nobeyama Millimeter Array toward an…
SMA CO(J=3-2) interferometric observations of the central region of M51
S. Matsushita, K. Sakamoto, C. -Y. Kuo +9
We present the first interferometric CO(J=3-2) observations (beam size of 3.9"x1.6" or 160pc x 65pc) with the Submillimeter Array (SMA) toward the center of the Seyfert 2 galaxy M5…
High Density Molecular Gas in the IR-bright Galaxy System VV114
Daisuke Iono, Paul T. P. Ho, Min S. Yun +3
New high resolution CO(3-2) interferometric map of the IR-bright interacting galaxy system VV114 observed with the Submillimeter Array (SMA) reveal a substantial amount of warm and…
Submillimeter Array Observations of CS J=14--13 Emission from the Evolved Star IRC+10216
K. H. Young, T. R. Hunter, D. J. Wilner +1
We present imaging observations of the evolved star IRC+10216 in the CS J=14--13 line at 685.4 GHz and associated submillimeter continuum at about 2'' resolution made with the part…
Submillimeter Array observations of ISM in starburst galaxies
Kazushi Sakamoto, Satoki Matsushita, Alison B. Peck +5
The Submillimeter Array (SMA) has been under construction at the 4100 m summit of Mauna Kea, Hawaii. The array is going to allow imaging of lines and continuum at sub-arcsecond res…