Interstellar high ionized absorptions in the Centaurus sky direction

Details Interstellar high ionized absorptions in the Centaurus sky direction Interstellar high ionized absorptions in the Centaurus sky direction

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.227f&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 227-229 (SEE N89

Astronomy and Astrophysics

Astronomy

1

Absorption Spectra, Centaurus Constellation, Gas Ionization, Interstellar Extinction, Interstellar Gas, Iue, Ultraviolet Astronomy, Ultraviolet Spectra, B Stars, Interstellar Space, Spaceborne Astronomy

Scientific paper

From a set of six early A and five late B stars, it is established that a interstellar absorption due to Si IV ions is present in the direction of Centaurus. The hot interstellar gas responsible for these absorptions could originate from a shock front produced by a supernova explosion in the Sco-Cen association passed through the cold local interstellar medium. Results based on IUE observations at high resolution are discussed.

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