The rate of the angular-momentum loss due to magnetic breaking, as derived from binary statistics

Details The rate of the angular-momentum loss due to magnetic breaking, as derived from binary statistics The rate of the angular-momentum loss due to magnetic breaking, as derived from binary statistics

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983obs...103..280r&link_type=abstract

The Observatory, vol. 103, p. 280-283 (1983)

Physics

18

Scientific paper

A small sample of short-period binary stars suggests that their
angular-momentum-loss (AML) rates are proportional to P-1.2.
AML rates of single slowly rotating stars depend much more on rotational
period (≡P-3). Extrapolations of AML rates from slow
rotators to rapidly rotating systems might be erroneous.

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