Highly ionized gas in the galactic halo

Details Highly ionized gas in the galactic halo Highly ionized gas in the galactic halo

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.176..435w&link_type=abstract

In ESA 3rd European IUE Conf. p 435-437 (SEE N83-11889 02-88)

Physics

1

Halos, Interstellar Gas, Ionized Gases, Milky Way Galaxy, Interstellar Extinction, Interstellar Matter, Iue, Resonance Lines, Ultraviolet Absorption

Scientific paper

Results of a study of CIV, Si IV and NV interstellar absorption lines in
IUE spectra of distant early stars in the halo of our galaxy are
summarized. The study detected CIV and Si IV lines towards approximately
two-thirds of the sample of 24 stars. The NV line, however, is only
detected towards two stars.

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