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Formation of a B0.5 Star Due to the Interaction of a Shock Wave with a Molecular Cloud in IC1805

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 93))

Abstract

An isolated B0.5 star has been observed, using radio techniques, in the optically obscured region ahead of a shock front which is propagating into a molecular cloud. The shock is driven chiefly by stellar winds from an OB-association. The method for detecting the star is described as well as the parameters for the region; some implications to star formation are given.

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© 1982 D. Reidel Publishing Company

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Hughes, V.A. (1982). Formation of a B0.5 Star Due to the Interaction of a Shock Wave with a Molecular Cloud in IC1805. In: Roger, R.S., Dewdney, P.E. (eds) Regions of Recent Star Formation. Astrophysics and Space Science Library, vol 93. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7778-5_47

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  • DOI: https://doi.org/10.1007/978-94-009-7778-5_47

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7780-8

  • Online ISBN: 978-94-009-7778-5

  • eBook Packages: Springer Book Archive

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