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A Survey of the M17SW Giant Molecular Cloud for H-alpha Emission Stars

Published online by Cambridge University Press:  04 August 2017

Masao Shinohara
Affiliation:
Komazawa University, Komazawa, Setegaya-ku, Tokyo 154, Japan
Katsuo Ogura
Affiliation:
Kokugakuin University, Higashi, Shibuya-ku, Tokyo 150, Japan

Extract

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The M17SW giant molecular cloud extends over 4° (∼ 160 pc) at the south-west of the giant H II region M17. The distance and the mass of the cloud are estimated to be approximately 2.2 kpc and 3x105 M, respectively.

Type
I. Star Forming Processes in the Solar Neighborhood
Copyright
Copyright © Reidel 1987 

References

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