Magnetic fields in late-type stars

Details Magnetic fields in late-type stars Magnetic fields in late-type stars

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mnras.197p..45k&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 197, Dec. 1981, p. 45P-49P. Research supported by the Alfred P. Sloan F

Astronomy and Astrophysics

Astronomy

44

Angular Velocity, Late Stars, Stellar Magnetic Fields, Stellar Rotation, Chromosphere, Convective Flow, Dwarf Stars, Dynamo Theory

Scientific paper

Observations show that magnetic activity in late-type stars is correlated with rotation rates and that there is a discontinuous change in behavior at a critical rotation period. This can be explained as a consequence of a transition from convection in rolls parallel to the rotation axis to normal convection cells as the angular velocity is decreased.

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