Anti-solar differential rotation

Details Anti-solar differential rotation Anti-solar differential rotation

2005-04-07

arxiv.org/abs/astro-ph/0504173v1

Astron.Nachr. 325 (2004) 496

Astronomy and Astrophysics

Astrophysics

5 pages, 6 figures, Astron. Nachr. 325, 496 (2004)

Scientific paper

10.1002/asna.200410297

The differential rotation of anti-solar type detected by observations for several stars may result from a fast meridional flow. The sufficiently intensive meridional circulation may be caused by large-scale thermal inhomogeneities or, perhaps, by tidal forcing from a companion star. First results of simulations of the anti-solar rotation of a giant star with magnetically induced thermal inhomogeneities are presented. Perspectives for observational check of the theory are discussed.

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