Hostname: page-component-7479d7b7d-k7p5g Total loading time: 0 Render date: 2024-07-11T06:28:33.750Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Braunsfurth, E., Rohlfs, K.: 1984, Astron. Astrophys. 57, 189.Google Scholar
Fürst, E., Reich, W., Reich, P., Sofue, Y., Handa, T.: 1985, Nature 314, 720 Google Scholar
Fürst, E. et al.: 1987, in preparationGoogle Scholar
Odegard, N.: 1986, Astron. J. 92, 1372 Google Scholar
Weiler, K.W.: 1983, The Observatory, 1054th editionGoogle Scholar