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A&A 373, 211-221 (2001)
DOI: 10.1051/0004-6361:20010600
Accretion physics of AM Herculis binaries
I. Results from one-dimensional stationary radiation hydrodynamics
A. Fischer and K. BeuermannUniversitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
(Received 30 November 2000 / Accepted 23 April 2001 )
Abstract
We have solved the one-dimensional stationary two-fluid
hydrodynamic equations for post-shock flows on accreting magnetic
white dwarfs simultaneous with the fully frequency and angle-dependent
radiative transfer for cyclotron radiation and bremsstrahlung.
Magnetic field strengths B = 10 to 100 MG are considered. At given
B, this theory relates the properties of the emission region to a
single physical parameter, the mass flow density (or accretion rate
per unit area)
. We present the normalized temperature
profiles and fit formulae for the peak electron temperature, the
geometrical shock height, and the column density of the post-shock
flow. The results apply to pillbox-shaped emission regions. With a
first-order temperature correction they can also be used for narrower
columns provided they are not too tall.
Key words: stars: cataclysmic variables -- stars: white dwarfs -- stars: binaries: close -- radiative transfer -- hydrodynamics
Offprint request: K. Beuermann, beuermann@uni-sw.gwdg.de
© ESO 2001
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