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G18.95-1.1, A Composite Supernova Remnant Interacting with the Ambient Interstellar Medium

Published online by Cambridge University Press:  12 April 2016

E. Fürst ,
W. Reich ,
E. Hummel  and
Y. Sofue
E. Fürst
Affiliation:
Max-Planck-Institut für Radloastronomie, Auf dem Hügel 69, D-5300 Bonn 1, F.R.G.
W. Reich
Affiliation:
Max-Planck-Institut für Radloastronomie, Auf dem Hügel 69, D-5300 Bonn 1, F.R.G.
E. Hummel
Affiliation:
Max-Planck-Institut für Radloastronomie, Auf dem Hügel 69, D-5300 Bonn 1, F.R.G.
Y. Sofue
Affiliation:
Department of Astronomy, Faculty of Science, University of Tokyo, Bunkyo-ku, Tokyo 113, Japan

Abstract

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New radio continuum and spectral line observations of the Galactic radio source G18.95-1.1 are reported. The distance to G18.95-1.1 is 2 kpc as derived from HI-21 cm spectral line observations. These data also indicate an interaction with the interstellar medium. The radio continuum observations classify G18.95-1.1 as a composite supernova remnant.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 253 - 256
Copyright
Copyright © Cambridge University Press 1988

References

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