EDP Sciences
Free Access
Volume 463, Number 2, February IV 2007
Page(s) 671 - 682
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361:20065224
Published online 23 November 2006

A&A 463, 671-682 (2007)
DOI: 10.1051/0004-6361:20065224

Rotational velocities of A-type stars

III. Velocity distributions
F. Royer1, J. Zorec2, and A. E. Gómez1

1  GEPI/CNRS UMR 8111, Observatoire de Paris, 5 place Jules Janssen, 92195 Meudon Cedex, France
    e-mail: frederic.royer@obspm.fr
2  CNRS, Institut d'Astrophysique de Paris, 98bis boulevard Arago, 75014 Paris, France

(Received 17 March 2006 / Accepted 22 October 2006 )

Aims.A sample of $v\sin i$ of B9 to F2-type main sequence single stars has been built from highly homogeneous $v\sin i$ parameters determined for a large sample cleansed of objects presenting the Am and Ap phenomenon as well as of all known binaries. The aim is to study the distributions of rotational velocities in the mass range of A-type stars for normal single objects.
Methods.Robust statistical methods are used to rectify the $v\sin i$ distributions for the projection effect and the error distribution. The equatorial velocity distributions are obtained for about 1100 stars divided in six groups defined by the spectral type, under the assumption of randomly orientated rotational axes.
Results.We show that late B and early A-type main-sequence stars have genuine bimodal distributions of true equatorial rotational velocities probably due to angular momentum loss and redistribution that the star underwent before reaching the main sequence. A striking lack of slow rotators is noticed among intermediate and late A-type stars.

Key words: stars: early-type -- stars: rotation

© ESO 2007

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