Hostname: page-component-cd9895bd7-gxg78 Total loading time: 0 Render date: 2024-12-26T13:11:30.697Z Has data issue: false hasContentIssue false
  • English
  • Français

Physical and chemical properties of the AFGL 333 cloud

Published online by Cambridge University Press:  01 August 2006

Takeshi Sakai ,
Tomoharu Oka  and
Satoshi Yamamoto
Takeshi Sakai
Affiliation:
Nobeyama, Radio Observatory, Japan email: sakai@nro.nao.ac.jp
Tomoharu Oka
Affiliation:
Department of Physics, Graduate School of Science, University of Tokyo, Japan
Satoshi Yamamoto
Affiliation:
Department of Physics, Graduate School of Science, University of Tokyo, Japan
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have found massive clumps without any sign of active star formation in the AFGL 333 cloud. We present a study of the physical and chemical properties of the AFGL 333 cloud.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 471
Copyright
Copyright © International Astronomical Union 2007

References

Sakai, T., Oka, T. & Yamamoto, S. 2006, ApJ 649, 268CrossRefGoogle Scholar
Thronson, H. A., Jr., Campbell, M. F. & Hoffmann, W. F. I. 1980, ApJ 239, 533CrossRefGoogle Scholar
Thronson, H. A., Jr., Lada, C. J. & Hewagama, T. 1985, ApJ 297, 662CrossRefGoogle Scholar