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Submillimeter CO Spectroscopy of Low Mass Young Stellar Objects

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Circumstellar Matter 1994

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Abstract

We report submillimeter CO(6-5) observations around 15 nearby young stellar objects of low mass. The correlation between linewidth and peak temperature indicates shock heating of dense gas, presumably at the origin of molecular outflows.

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Author information

Authors and Affiliations

  1. Max-Planck-Institut für extraterrestrische Physik, Postfach 1603, 85740, Garching, Germany

    K. F. Schuster, A. P. G. Russell & A. I. Harris

  2. Now IRAM Grenoble, France

    K. F. Schuster

  3. Now ROE Edinburgh, Scotland

    A. P. G. Russell

  4. Now FCRAO UMass, Amherst, USA

    A. I. Harris

Authors
  1. K. F. Schuster
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  2. A. P. G. Russell
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  3. A. I. Harris
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Editor information

G. D. Watt P. M. Williams

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© 1995 Springer Science+Business Media Dordrecht

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Schuster, K.F., Russell, A.P.G., Harris, A.I. (1995). Submillimeter CO Spectroscopy of Low Mass Young Stellar Objects. In: Watt, G.D., Williams, P.M. (eds) Circumstellar Matter 1994. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0147-9_22

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  • DOI: https://doi.org/10.1007/978-94-011-0147-9_22

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-4066-2

  • Online ISBN: 978-94-011-0147-9

  • eBook Packages: Springer Book Archive

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