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Submillimeter CO spectroscopy of low mass young stellar objects

  • Session B: Pre-Main Sequence Outflows
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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 notes

  1. K. -F. Schuster

    Present address: Now IRAM Grenoble, France

  2. A. P. G. Russell

    Present address: Now ROE Edinburgh, Scotland, U.K.

  3. A. I. Harris

    Present address: Now FCRAO UMass, Amherst, USA

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

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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Schuster, K.F., Russell, A.P.G. & Harris, A.I. Submillimeter CO spectroscopy of low mass young stellar objects. Astrophys Space Sci 224, 117–120 (1995). https://doi.org/10.1007/BF00667833

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  • DOI: https://doi.org/10.1007/BF00667833

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