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A CO (J = 1-0) Survey of Five Supernova Remnants at ℓ = 70° - 110°

Published online by Cambridge University Press:  12 April 2016

Y. Fukui  and
K. Tatematsu
Y. Fukui
Affiliation:
Department of Astrophysics, Faculty of Science, Nagoya University, Chikusa-ku, Nagoya 464, Japan
K. Tatematsu
Affiliation:
Department of Astrophysics, Faculty of Science, Nagoya University, Chikusa-ku, Nagoya 464, Japan

Abstract

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A program of CO observations of five selected supernova remnants is in progress on the 4-m radio telescope at Nagoya. Here, we report observations of two supernova remnants, G78.2+2.1 (the γ Cygni SNR) and HB21. In these two remnants we have obtained evidence for the interaction between the supernova remnants and molecular gas.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 261 - 264
Copyright
Copyright © Cambridge University Press 1988

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