Statistical Study of Axial Rotation in A Type Stars with New Determination of v sin i

Details Statistical Study of Axial Rotation in A Type Stars with New Determination of v sin i Statistical Study of Axial Rotation in A Type Stars with New Determination of v sin i

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..275g&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Stellar Rotation, Stars: A Type

Scientific paper

We have observed all A type stars of the southern hemisphere brighter
than 6.5 mag in order to perform statistical studies of axial rotation.
The spectra were obtained at the 2.15 m telescope at CASLEO. We have
used the method of Diaz et al. (2011) to calculate axial rotation
velocities.

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