Discrete absorption components and stellar wind features in spectra of Beta ORI

Details Discrete absorption components and stellar wind features in spectra of Beta ORI Discrete absorption components and stellar wind features in spectra of Beta ORI

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.281b.151b&link_type=abstract

In ESA, Proceedings of the Celebratory Symposium on a Decade of UV Astronomy with the IUE Satellite, Volume 2 p 151-154 (SEE N89

Astronomy and Astrophysics

Astronomy

1

B Stars, Iue, Spaceborne Astronomy, Stellar Winds, Ultraviolet Absorption, Ultraviolet Astronomy, Ultraviolet Spectra, Stellar Mass Ejection, Stellar Models, Stellar Spectra, Time Dependence, Wind Velocity

Scientific paper

Stellar wind features and discrete absorption components (DAC) in
spectra of Beta Ori (B8Ia) were identified by comparing spectra obtained
at times of quite different mass loss. Recent observations provide data
on velocity-time dependence for DAC which are discussed in terms of the
applicability of the gas parcel model to late-B supergiants.

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