Other
Scientific paper
Jul 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002an....323..395g&link_type=abstract
Astronomische Nachrichten, vol. 323, no. 3/4, p. 395-398
Other
6
Stars: Spots, Magnetic Flux Tubes, Mhd, Stars: Evolution
Scientific paper
Star spots have been shown to exist on a variety of stars. The growing number of observed star spot distributions on different stars - though snapshot-like - may allow the derivation of a fundamental dependency of spot patterns on stellar parameters. This paper tries to establish a connection of generic stellar parameters with the latitude of star spots based on a numerical thin-flux-tube-evolution model. The model is applied to stars with masses between 0.4 and 4.0 M_sun at evolutionary stages from PMS to early giant stages. All model stars considered have an outer convection zone with a radiative core underneath. It is shown that the rotational period is the dominant parameter in determining the star-spot latitude. Another important factor is the fractional size of the radiative core, while the evolutionary stage and the stellar mass play only a minor role.
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