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A&A 389, 485-493 (2002)
DOI: 10.1051/0004-6361:20020622
Distortion of secondaries in semi-detached binaries and the cataclysmic variable period minimum
V. Renvoizé1, I. Baraffe1, 2, U. Kolb3 and H. Ritter21 C.R.A.L (UMR 5574 CNRS), École Normale Supérieure, 69364 Lyon Cedex 07, France
e-mail: vrenvoiz, ibaraffe@ens-lyon.fr
2 Max-Planck Institut für Astrophysik, Karl-Schwarzschild-str.1, 85741 Garching, Germany
e-mail: hsr@mpa-garching.mpg.de
3 Department of Physics & Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA, UK
e-mail: u.c.kolb@open.ac.uk
(Received 27 December 2001 / Accepted 15 April 2002 )
Abstract
Based on SPH simulations,
we quantify the geometrical distortion effect due to tidal and rotational
forces on polytropic secondaries in semi-detached binaries.
The main effect is an expansion of the polytropic star, with an effect
on the radius of ~5%-12%,
depending on the
polytropic index and the mass ratio. We apply such distortion
effects to the secular evolution of secondaries in
cataclysmic variable systems. We focus on systems below
the 2-3 h period gap and that approach
the minimum period. We find
a significant increase of the predicted minimum period (~4% if changes in the secondary's thermal relaxation are approximately
taken into account).
Though an improvement, the effect is not big enough to
solve the mismatch between predicted and observed minimum period
at 80 min.
Key words: stars: binaries: close -- stars: low-mass, brown dwarfs -- stars: evolution -- stars: novae, cataclysmic variables
Offprint request: V. Renvoizé, vrenvoiz@ens-lyon.fr
© ESO 2002
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