IUE absorption line studies of highly ionized interstellar gas

Details IUE absorption line studies of highly ionized interstellar gas IUE absorption line studies of highly ionized interstellar gas

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349....3s&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 3-16 (SEE N85-20961 11-8

Astronomy and Astrophysics

Astronomy

8

Absorption Spectra, Hot Stars, Interstellar Gas, Iue, Oao 3, Ultraviolet Astronomy, Combination, Extraterrestrial Radiation, H Ii Regions, Ionization Cross Sections, Line Spectra, Photoionization, Reaction

Scientific paper

IUE high dispersion echelle spectra of galactic and extragalactic sources have generally revealed the presence of absorption by interstellar Si IV and C IV. Occasionally N V has been detected. The observational results relating to these species will be reviewed for H II regions, supernova remnants, galactic disk gas, galactic halo gas, and extragalactic gas. For the various regions, the likely origin of the ionization is considered.

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