The influence of rotation and stellar winds upon the Be phenomenon

Details The influence of rotation and stellar winds upon the Be phenomenon The influence of rotation and stellar winds upon the Be phenomenon

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..777m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Oct. 1975, p. 777-784.

Astronomy and Astrophysics

Astronomy

33

B Stars, H Alpha Line, Stellar Rotation, Stellar Winds, Angular Velocity, Astronomical Catalogs, Early Stars, Radiation Pressure, Stellar Spectrophotometry

Scientific paper

A number of rapidly rotating B stars, not previously known as Be stars, were observed spectroscopically at H alpha. These results were then combined with existing data to show that the spectral type of a star and the minimum velocity at which it must rotate in order to become a Be star are related. The trend of this relationship is found to have a natural explanation in terms of stellar winds.

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