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Panel Discussion: The CO/H2 Abundance Ratio

Published online by Cambridge University Press:  07 August 2017

E.F. Van Dishoeck ,
A.E. Glassgold ,
M. Guélin ,
D.T. Jaffe ,
D.A. Neufeld ,
A.G.G.M. Tielens  and
C.M. Walmsley
E.F. Van Dishoeck
Affiliation:
Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands
A.E. Glassgold
Affiliation:
Dept. of Physics, New York Univ., New York 10003, USA
M. Guélin
Affiliation:
IRAM, Univ. de Grenoble, 38406 St. Martin-d'Hères, France
D.T. Jaffe
Affiliation:
Dept. of Astronomy, Univ. of Texas, Austin, TX 78712, USA
D.A. Neufeld
Affiliation:
Dept. of Astronomy, Johns Hopkins Univ., Baltimore, MD 21218, USA
A.G.G.M. Tielens
Affiliation:
NASA-Ames Res. Center 245-3, Moffett Field, CA 94035, USA
C.M. Walmsley
Affiliation:
MPI für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Germany

Abstract

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The observational and theoretical information on the CO/H2 abundance in a variety of astrophysical regions including diffuse clouds, dense star-forming regions, shocked gas and circumstellar envelopes is discussed and reviewed.

Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 285 - 295
Copyright
Copyright © Kluwer 1992 

References

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