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The Interaction of the Supernova Remnant VRO 42.05.01 with its HI Environment

Published online by Cambridge University Press:  12 April 2016

T.L. Landecker ,
S. Pineault ,
D. Routledge  and
J.F. Vaneldik
T.L. Landecker
Affiliation:
Dominion Radio Astrophysical Observatory, Penticton, B.C.
S. Pineault
Affiliation:
Département de physique, Université Laval, Québec, P.Q.
D. Routledge
Affiliation:
Electrical Engineering Dept., University of Alberta, Edmonton, Alberta
J.F. Vaneldik
Affiliation:
Electrical Engineering Dept., University of Alberta, Edmonton, Alberta

Abstract

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VRO 42.05.01 (G166.0+4.3) is a SNR which has broken into and re-energized an old interstellar cavity. Observations of HI in a field containing the SNR show features associated with it. An expanding shell of mass ∼40 M⊙ is associated with the semi-circular shell of the SNR. The cavity, which the SNR has re-energized, is seen in the HI. A cloud of HI of mass ∼25 M⊙ has apparently been hit by the shock and has been accelerated by the post-shock flow.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 245 - 248
Copyright
Copyright © Cambridge University Press 1988

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