Hostname: page-component-745bb68f8f-f46jp Total loading time: 0 Render date: 2025-01-14T17:20:19.366Z Has data issue: false hasContentIssue false
  • English
  • Français

A Statistical Study of the Correlation of Galactic Supernova Remnants and Spiral Arms

Published online by Cambridge University Press:  12 April 2016

Zongwei Li ,
J. Craig Wheeler ,
Frank N. Bash  and
William H. Jefferys
Zongwei Li
Affiliation:
(, Beijing Normal University)
J. Craig Wheeler
Affiliation:
The University of Texas at Austin Austin, Texas 78712
Frank N. Bash
Affiliation:
The University of Texas at Austin Austin, Texas 78712
William H. Jefferys
Affiliation:
The University of Texas at Austin Austin, Texas 78712

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.

A statistical study of the correlation of Galactic supernova remnants with spiral arms and the disk is presented. SNR apparently have a larger radial scale length than disk stars. We estimate that only about 10 percent of the Galactic SNR have been detected.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 485 - 488
Copyright
Copyright © Cambridge University Press 1988

References

Blitz, L. et al. 1982, Ap. J., 49, 183.Google Scholar
Georgelin, Y.M. and Georgelin, Y.P. 1976, Astron. & Ap., 49, 57.Google Scholar
Green, D.A. 1984, M.N.R.A.S., 209, 449 CrossRefGoogle Scholar
Milne, D.K. 1979, Aust. J. Phys., 32, 83.CrossRefGoogle Scholar
van den Bergh, S. 1983, I.A.U. Symposium, No. 101.Google Scholar