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CO Observations of 2nd quadrant IRAS Sources

  • Part I: The Physics of Interstellar Molecular Clouds: Overview
  • 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))

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Abstract

Systematic observation of strong second quadrant IRAS sources at low resolution has revealed a surprising number of broad wings frequently associated with other clouds along the same line of sight as the IRAS source but undetected by IRAS.

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Authors and Affiliations

  1. Section de Meudon, DEMIRM, Observatoire de Paris, F-92195, Meudon cedex

    J. Braine & F. Combes

  2. Radioastronomie Millimétrique, ENS, 24 Rue Lhomond, F75231, Paris cedex 05

    C. Dupraz, F. Casoli, F. Combes & M. Gérin

Authors
  1. J. Braine
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  2. C. Dupraz
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  3. F. Casoli
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  4. F. Combes
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  5. M. Gérin
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© 1989 Springer-Verlag Berlin Heidelberg

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Braine, J., Dupraz, C., Casoli, F., Combes, F., Gérin, M. (1989). CO Observations of 2nd quadrant IRAS Sources. 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/BFb0119464

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  • DOI: https://doi.org/10.1007/BFb0119464

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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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