Stellar rotational velocities from the V sin i observations - Inversion procedures and applications to open clusters

Details Stellar rotational velocities from the V sin i observations - Inversion procedures and applications to open clusters Stellar rotational velocities from the V sin i observations - Inversion procedures and applications to open clusters

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26a...269..267g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 269, no. 1-2, p. 267-281.

Mathematics

Probability

40

Open Clusters, Radial Velocity, Stellar Rotation, T Tauri Stars, Probability Distribution Functions, Velocity Distribution

Scientific paper

We computed the distributions of the apparent rotational velocities in several open clusters. Then we showed that various inversion procedures are usable in the study of rotational velocities and we applied these procedures to the previous observed distributions. We found that the distribution of rotational velocities for stars hotter than 7000 K is uniform while it is peaked below. These results are compatible with the ones found for T Tauri stars.

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