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IUE Observations of the Gaseous Component of the Local Interstellar Medium

Published online by Cambridge University Press:  12 April 2016

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

Abstract

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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).

Type
Ultraviolet and EUV Absorption Studies
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 385390.Google Scholar
Gilra, D.P., Pwa, T.H., and Arnal, E.M. 1982b, in ibid, pp 391397.Google Scholar
Gilra, D.P. 1982, in ibid, pp 139141.Google Scholar