Rotational Velocities of Late-Type Stars

Details Rotational Velocities of Late-Type Stars Rotational Velocities of Late-Type Stars

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pasp..109..514f&link_type=abstract

Publications of the Astronomical Society of the Pacific, v.109, p.514-523

Astronomy and Astrophysics

Astronomy

180

Stars: Late-Type, Stars: Rotation

Scientific paper

A calibration based on the results of Gray has been used to determine projected rotational velocities for 133 bright stars with spectral types of F, G, or K, most of which appear in {\it The Bright Star Catalogue}. The vast majority have {\it v} sin {\it i} $\leq$ 10 km s$^{-1}$ and, thus, are slow rotators. With the new calibration, projected rotational velocities have been determined for a sample of 111 late-type stars, most of which are chromospherically active. Some of the stars have had their rotational velocities measured for the first time. (SECTION: Stars)

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