A Non-Empirical Rotation-Activity Relation for RS CVn Binaries Using Radio Luminosities

Details A Non-Empirical Rotation-Activity Relation for RS CVn Binaries Using Radio Luminosities A Non-Empirical Rotation-Activity Relation for RS CVn Binaries Using Radio Luminosities

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998iraj...25...33g&link_type=abstract

Irish Astronomical Journal, 1998, 25(1), 33

Astronomy and Astrophysics

Astronomy

2

Scientific paper

An analysis of a comprehensive survey of radio luminosities for RS CVn binary systems is given. A comparison is made between the rotation-activity correlations found using the usual semi-empirical Rossby number and a Rossby number deduced from detailed convection zone models. The use of a non-empirically derived Rossby number does not significantly improve the rotation-activity correlation. Although there are some indications that the rotation-activity correlations are marginally better for theoretically derived convective parameters this study is limited by the size of the sample.

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