On the UV spectra of Beta Carinae and Delta Velorum

Details On the UV spectra of Beta Carinae and Delta Velorum On the UV spectra of Beta Carinae and Delta Velorum

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....54..883s&link_type=abstract

Astronomy and Astrophysics, vol. 54, no. 3, Feb. 1977, p. 883-887.

Astronomy and Astrophysics

Astrophysics

4

A Stars, Computer Techniques, Early Stars, Stellar Spectra, Turbulence Effects, Ultraviolet Spectra, Optical Thickness, Spectrum Analysis, Stellar Atmospheres, Stellar Models, Stellar Rotation, Stellar Spectrophotometry

Scientific paper

Synthetic spectra have been computed and compared with the S59
observations of Beta Carinae (Al IV) and Delta Velorum (AOV). The
microturbulences determined for these fairly rapidly rotating stars do
not appear to be higher than in slow rotators of similar spectral type
although there is some suggestion that it increases with optical depth.

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