The period gap and masses of cataclysmic variables

Details The period gap and masses of cataclysmic variables The period gap and masses of cataclysmic variables

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...248..525h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 248, no. 2, Aug. 1991, p. 525-530.

Astronomy and Astrophysics

Astrophysics

16

Cataclysmic Variables, Stellar Evolution, Stellar Mass Ejection, Stellar Magnetic Fields, Stellar Models, Stellar Orbits, White Dwarf Stars

Scientific paper

Consequences of the currently-favored view that the cataclysmic variable period gap results from a sharp decrease in orbital braking once the secondary becomes fully convective are examined. It is shown that the period distribution of systems near the edge of the gap imposes, for a given stellar model, tight constraints on the parameters of the Mestel-Spruit magnetic braking law. The white dwarf mass M1 in systems such as TU Men or YZ Cnc must be high, unless these systems are assumed coincidentally to have been born close to the upper edge of the gap. With the present adopted parameters, M1 of not less than 1 solar mass is predicted for both systems. Observational mass determination for these systems and those which should be discovered by Rosat thus offer a stringent test of current theories of the period gap. It is shown that, depending on the secondary mass and age when it first comes into contact, evolution can be driven by angular momentum losses either through magnetic braking or gravitational radiation, and that for periods greater than 2.5-2.6 h, high mass transfer rates are possible, as observed in V795 Her.

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