Hostname: page-component-6bb9c88b65-dwch4 Total loading time: 0 Render date: 2025-07-26T14:30:54.228Z Has data issue: false hasContentIssue false
  • English
  • Français

IUE Observations of the Gaseous Component of the Local Interstellar Medium

Published online by Cambridge University Press:  12 April 2016

Daya P. Gilra
Daya P. Gilra*
Affiliation:
S M Systems and Research Corporation Lanham, Md. 20706, U.S.A.

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.

Discovery of interstellar Ge, Ga, and Kr is reported. Several intercombination lines of Fe II are detected. The depletion is most pronounced in Ca, Ti, and V. The highly ionized gas C IV and Si IV is not coextensive with the Si II and C II gas nor with the 0 VI gas. The molecular gas (CO) shows very small velocity dispersion (b~l km/sec).

Information

Type
Ultraviolet and EUV Absorption Studies
Information
International Astronomical Union Colloquium , Volume 81: Local Interstellar Medium , 1984 , pp. 89 - 90
Copyright
Copyright © NASA 1984

References

Gilra, D.P., Pwa, T.H., Arnal, E.M., and Vries, J.de 1982a, in Proceedings of the Third European IUE Conference, Madrid, ESA Special Publication, ESA SP 176. pp 385–390.Google Scholar
Gilra, D.P., Pwa, T.H., and Arnal, E.M. 1982b, in ibid, pp 391–397.Google Scholar
Gilra, D.P. 1982, in ibid, pp 139–141.Google Scholar