Circumstellar material around rapidly rotating B stars. I - Nonemission-line stars

Details Circumstellar material around rapidly rotating B stars. I - Nonemission-line stars Circumstellar material around rapidly rotating B stars. I - Nonemission-line stars

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..997o&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Dec. 1982, p. 997-1000.

Astronomy and Astrophysics

Astronomy

3

Absorption Spectra, B Stars, Line Spectra, Stellar Envelopes, Stellar Rotation, Ultraviolet Spectra, Emission Spectra, Fine Structure, Iron, Low Speed, Oxygen, Silicon, Stellar Mass Ejection, Stellar Spectrophotometry

Scientific paper

Evidence of low-velocity circumstellar material around a number of rapidly rotating nonemission-line B stars is sought. No evidence is found for circumstellar shell lines in any of the stars observed. If circumstellar material is present, then these results place constraints on the physical properties of the envelope. Furthermore, contamination of interstellar line profiles with circumstellar components in rapidly rotating non-Be stars is, in general, negligible.

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