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Molecular Clouds in the Central 100-pc of the Galactic Center

Published online by Cambridge University Press:  23 September 2016

M. Tsuboi ,
T. Handa ,
M. Inoue ,
J. Inatani  and
N. Ukita
M. Tsuboi
Affiliation:
Nobeyama Radio Observatory, Minamisaku Nagano 384–13, Japan
T. Handa
Affiliation:
Nobeyama Radio Observatory, Minamisaku Nagano 384–13, Japan
M. Inoue
Affiliation:
Nobeyama Radio Observatory, Minamisaku Nagano 384–13, Japan
J. Inatani
Affiliation:
Nobeyama Radio Observatory, Minamisaku Nagano 384–13, Japan
N. Ukita
Affiliation:
Nobeyama Radio Observatory, Minamisaku Nagano 384–13, Japan

Abstract

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We have observed CS (J=1–0/2–1) lines in a 60′×30′(1×b) area of the Galactic center region. There are two large-scale features with elliptical shape in the position–velocity maps, which suggest shell–like structures in the region. One is the ring with a radius of ~40 pc in the positive galactic latitude region and another is the shell with a radius of ~20 pc in the negative galactic longitude region. These could be due to suggest star bursts occurred in the Galactic center region.

Type
The Large - Scale Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 136: The Galactic Center , 1989 , pp. 135 - 140
Copyright
Copyright © Kluwer 1989 

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