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IC 443: The Interaction of a SNR with a Molecular Cloud

Published online by Cambridge University Press:  12 April 2016

Michael G. Burton
Michael G. Burton*
Affiliation:
NASA Ames MS 245-6, Moffett Field, California 94035USA

Abstract

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Observations are presented of shocked line emission from H2, CO and HCO+ molecules in the SNR IC 443. IC 443 is the most luminous galactic H2 emission line source yet discovered. The implications for physical processes in shocked molecular gas are discussed.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 399 - 402
Copyright
Copyright © Cambridge University Press 1988

References

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