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Triggered star formation within the bright-rimmed cloud SFO 75

Published online by Cambridge University Press:  01 August 2006

J. S. Urquhart ,
M. A. Thompson ,
L. K. Morgan  and
Glenn J. White
J. S. Urquhart
Affiliation:
School of Physics and Astrophysics, University of Leeds, Leeds, LS2 9JT, UK email: jsu@ast.leeds.ac.uk
M. A. Thompson
Affiliation:
Centre for Astrophysics Research, Science and Technology Research Institute, University of Hertfordshire, College Lane, Hatfield, AL10 9AB, UK
L. K. Morgan
Affiliation:
Green Bank Telescope, P.O. Box 2, Green Bank, WV 24944, USA
Glenn J. White
Affiliation:
Dept. of Physics & Astronomy, The Open University, Walton Hall, Milton Keynes, MK7 6AA, UK Space Physics Division, Space Science & Technology Division, CCLRC Rutherford Appleton Laboratory, Chilton, Didcot, Oxfordshire, OX11 0QX, UK
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Abstract

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We present the results of a multi-wavelength line and continuum study of the bright-rimmed cloud SFO 75 in an attempt to determine whether the ionisation front and its associated shocks, driven by the nearby O star, have triggered the formation of a new generation of stars within this bright-rimmed cloud.

Keywords

Radio continuum: stars – Stars: formation – Stars: pre-main sequence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 483
Copyright
Copyright © International Astronomical Union 2007

References

Sugitani, K. & Ogura, K. 1994, ApJS 92, 163Google Scholar
Thompson, M. A., Urquhart, J. S. & White, G. J. 2004, A&A 415, 627Google Scholar
Urquhart, J. S., Thompson, M. A., Morgan, L. K., & White, G. J. 2006, A&A 450, 625Google Scholar