A statistical method of estimating the rotation of Be stars

Details A statistical method of estimating the rotation of Be stars A statistical method of estimating the rotation of Be stars

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cha%26a..11...10c&link_type=abstract

Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 11, March 1987, p. 10-14. Translation.

Astronomy and Astrophysics

Astrophysics

5

B Stars, Statistical Analysis, Stellar Rotation, Angular Velocity, Axes Of Rotation, Critical Velocity

Scientific paper

The paper presents a statistical method which will estimate the true
rotational velocity v of a Be star from its observed apparent velocity u
= Vsini. It is shown that Be stars do not rotate with the critical
velocity and that the ratio between their real velocity and the critical
velocity is about 0.7.

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