Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-23T02:04:39.359Z Has data issue: false hasContentIssue false
  • English
  • Français

A sample of star forming regions triggered by cloud-cloud collision

Published online by Cambridge University Press:  01 August 2006

Bei Xin  and
Jun-Jie Wang
Bei Xin
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China. e-mail: [email protected] and [email protected]
Jun-Jie Wang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China. e-mail: [email protected] and [email protected]
Rights & Permissions [Opens in a new window]

Extract

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.

Collision between molecular clouds is considered an efficient mechanism to trigger cloud collapse to form stars. Various observations show that the process is taking place in the universe (Vallee 1995; Wang et al. 2004).

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 498
Copyright
Copyright © International Astronomical Union 2007

References

Vallee, J.P. 1995, AJ 110, 2256CrossRefGoogle Scholar
Wang, J.J., Chen, W.P., Miller, M., Qin, S.L. & Wu, Y.F. 2004, ApJ 614, L105CrossRefGoogle Scholar
Yang, J., Jiang, Z.B., Wang, M., Ju, B.G. & Wang, H.C. 2002, ApJS 141, 157CrossRefGoogle Scholar
Zhou, S., Evans, N.J., II, Koempe, C. & Walmsley, C.M. 1993, ApJ 404, 232CrossRefGoogle Scholar