The theoretical spread of the main sequence due to stellar rotation

Details The theoretical spread of the main sequence due to stellar rotation The theoretical spread of the main sequence due to stellar rotation

Feb 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983obs...103....8c&link_type=abstract

The Observatory, vol. 103, p. 8-12 (1983)

Physics

5

Scientific paper

The rotational spread of the main sequence is shown to depend strongly
on the internal angular-velocity distribution. Two parameters may be
enough to describe this distribution, but observations do not yet
strongly constrain these parameters.

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