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Molecular cloud evolution and star formation

  • Part I: The Physics of Interstellar Molecular Clouds: Theory
  • Conference paper
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The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 331))

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Abstract

The origin and growth of molecular clouds is described and mechanisms for molecular cloud support are reviewed. Cloud disruption is discussed with emphasis on star formation efficiency. Issues pertaining to massive star enhanced star formation are summarized, and a mechanism for bimodal star formation is presented. Applications are made to the global star formation rate and to starburst galaxies.

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© 1989 Springer-Verlag Berlin Heidelberg

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Silk, J. (1989). Molecular cloud evolution and star formation. In: The Physics and Chemistry of Interstellar Molecular Clouds: mm and Sub-mm Observations in Astrophysics. Lecture Notes in Physics, vol 331. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0119503

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  • DOI: https://doi.org/10.1007/BFb0119503

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-51297-4

  • Online ISBN: 978-3-540-46187-6

  • eBook Packages: Springer Book Archive

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