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Infrared Molecular Spectroscopy of Orion

Published online by Cambridge University Press:  07 August 2017

Neal J. Evans II
Neal J. Evans II*
Affiliation:
Astronomy Department, The University of Texas, Austin Texas 78712, USA E-mail [email protected]

Abstract

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Recent results on infrared spectroscopy of the cluster of sources in the Orion molecular cloud are discussed. These results imply very high abundances of CO, C2H2, HCN, and OCS, suggesting that grain surface chemistry has been important.

Type
Quiescent Clouds and Regions of Star Formation
Information
Symposium - International Astronomical Union , Volume 150: Astrochemistry of Cosmic Phenomena , 1992 , pp. 265 - 269
Copyright
Copyright © Kluwer 1992 

References

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