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Triggered Star Formation from Bubbles S51, N68, and N131

Published online by Cambridge University Press:  21 March 2013

C. P. Zhang  and
J. J. Wang
C. P. Zhang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, PR China; email: zcp0507@gmail.com
J. J. Wang
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, PR China; email: zcp0507@gmail.com
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Abstract

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We investigated the environment of the infrared dust bubbles S51 (Zhang & Wang 2012a), N68 (Zhang & Wang 2012b), and N131 (Zhang et al. 2012) from catalogue of Churchwell et al. (2006), and searched for evidence of triggered star formation.

Keywords

infrared: stars — stars: formation — ISM: bubbles — HII regions
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 65
Copyright
Copyright © International Astronomical Union 2013

References

Churchwell, E., Povich, M. S., Allen, D., et al. 2006, ApJ, 649, 759Google Scholar
Lo, N., Cunningham, M. R., Jones, P. A., et al. 2009, MNRAS, 395, 1021CrossRefGoogle Scholar
Zhang, C. P. & Wang, J. J. 2012a, A&A, 544, A11Google Scholar
Zhang, C.-P. & Wang, J.-J. 2012b, arXiv:1208.0423Google Scholar
Zhang, C.-P., Wang, J.-J., & Xu, J.-L. 2012, A&A, SubmittedGoogle Scholar