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A non-circumstellar origin of the hump

  • Part II: The Chemistry of Interstellar Molecular Clouds
  • Conference paper
  • First Online:
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))

  • 142 Accesses

Abstract

The particles responsible for the 217.5 nm interstellar extinction feature may originate from photoprocessed organic material on dust grains.

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Authors and Affiliations

  1. Laboratory for Astrophysics, P.O. 9504, 2300 RA, Leiden, The Netherlands

    P.M.M. Jenniskens & M.S. De Groot

Authors
  1. P.M.M. Jenniskens
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  2. M.S. De Groot
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© 1989 Springer-Verlag Berlin Heidelberg

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Jenniskens, P., De Groot, M. (1989). A non-circumstellar origin of the hump. 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/BFb0119517

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  • DOI: https://doi.org/10.1007/BFb0119517

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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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