Hostname: page-component-84b7d79bbc-rnpqb Total loading time: 0 Render date: 2024-07-29T03:00:00.186Z Has data issue: false hasContentIssue false
  • English
  • Français

HI Associated with Cas A

Published online by Cambridge University Press:  12 April 2016

W.M. Goss ,
P.M.W. Kalberla  and
U.J. Schwarz
W.M. Goss
Affiliation:
NRAO, Socorro, New Mexico
P.M.W. Kalberla
Affiliation:
Radio Astronomy Institute, Bonn, Federal Republic of Germany
U.J. Schwarz
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands

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 small HI absorption feature has been detected in front of Cas A at a velocity of -66 km/s. This HI feature can probably be associated with a recombined high density QSF.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 239 - 243
Copyright
Copyright © Cambridge University Press 1988

References

Bell, A.R.: 1977, Monthly Notices Roy. Astron. Soc. 179, 573.Google Scholar
Braun, R.: 1987, Astron. Astrophys. 171, 233.Google Scholar
Braun, R., Strom, R.G.: 1986, Astron. Astrophys. Suppl., 63, 345.Google Scholar
McKee, C.F., Cowle, L.L.: 1975, Astrophys. J. 195, 715 Google Scholar
Mebold, U., Hills, D.L.: 1975, Astron. Astrophys. 42, 187.Google Scholar
van den Bergh, S., Kamper, K.W.: 1983, Astrophys. J. 268, 129.Google Scholar
van den Bergh, S., Kamper, K.W.: 1985, Astrophys. J. 293, 537 (vdBK).CrossRefGoogle Scholar