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Radiation driven implosion model for star formations near an H II region

Published online by Cambridge University Press:  01 August 2006

K. Motoyama ,
T. Umemoto  and
H. Shang
K. Motoyama
Affiliation:
Theoretical Institute for Advanced Research in Astrophysics, Hsin-Chu, 300, Taiwan
T. Umemoto
Affiliation:
National Astronomical Observatory, Mikata, Tokyo 181-8588, Japan
H. Shang
Affiliation:
Theoretical Institute for Advanced Research in Astrophysics, Hsin-Chu, 300, Taiwan Academia Sinica Institute of Astronomy and Astrophysics, P.O. Box 23-141, 106, Taiwan
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Abstract

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We performed numerical simulation including UV radiation transfer, and investigated effects of radiation driven implosion on star formation processes. We also observed two bright-rimmed clouds with C12O(J=1-0) and C13O(J=1-0) in order to compare density distributions between numerical results and observational results. Density profiles of bright-rimmed clouds are consistent with those of numerical simulations. These facts insist that star formations in bright-rimmed clouds are triggered by radiation driven implosion.

Keywords

radiation driven implosionbright-rimmed clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 450
Copyright
Copyright © International Astronomical Union 2007

References

Bertoldi, F. 1989, ApJ 346, 735Google Scholar