Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.289...59z&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 289, Issue 1, pp. 59-65.
Astronomy and Astrophysics
Astronomy
17
Binaries: Close, Stars: Evolution, Stars: Magnetic Fields, Stars: Mass-Loss, Novae, Cataclysmic Variables
Scientific paper
We show how a combination of two alpha-Omega dynamos, one in the convective envelope and the other at the boundary with a slowly rotating radiative core, can nicely explain the secular evolution of cataclysmic variables. The boundary-layer dynamo is dominant when the convective core is small. There it drives magnetic braking which leads to mass-transfer rates of the order of 10^-9M/yr^-1. When the star becomes fully convective, this dynamo switches off. This allows the star to contract inside its Roche lobe creating a period gap at about 3h. The envelope dynamo is dominant at larger periods, while its effects are comparable with gravitational radiation below 3h. It does not, therefore, have much effect on the edges of the period gap. The boundary-layer dynamo must maintain a universal rate of angular momentum loss for all cataclysmic variables if it is to produce the well-defined, observed period gap. The envelope dynamo, on the other hand, may fluctuate considerably and hence give rise to the wide range of mass-transfer rates implied for systems away from the period gap.
Bianchini Antonio
Tout Christopher A.
Zangrilli Luca
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