Volume 491, Number 2, November IV 2008
|Page(s)||525 - 529|
|Section||Stellar structure and evolution|
|Published online||23 September 2008|
Influence of Compton scattering on the broad-band X-ray spectra of intermediate polars
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany e-mail: firstname.lastname@example.org
2 Kazan State University, Kremlevskaja str. 18, Kazan 420008, Russia
3 Astronomy Division, Department of Physical Sciences, PO Box 3000, 90014 University of Oulu, Finland
4 CEA Saclay, DSM/DAPNIA/Service d'Astrophysique (CNRS FRE 2591), 91191 Gif-sur-Yvette, France
5 AIM, UMR 7158, CEA - CNRS - Université Paris 7, France
Accepted: January 1900
Context. The majority of cataclysmic variables observed in the hard X-ray energy band are intermediate polars where the magnetic field is strong enough to channel the accreting matter to the magnetic poles of the white dwarf. A shock above the stellar surface heats the gas to fairly high temperatures (10–100 keV). The post-shock region cools mostly via optically thin bremsstrahlung.
Aims. We investigate the influence of Compton scattering on the structure and the emergent spectrum of the post-shock region. We also study the effect it has on the mass of the white dwarfs obtained from fitting the observed X-ray spectrum of intermediate polars.
Methods. We construct the model of the post-shock region taking Compton scattering into account. The radiation transfer equation is solved in the plane-parallel approximation. The feedback of Compton scattering on the structure of the post-shock region is also accounted for. A set of the post-shock region model spectra for various white dwarf masses is calculated.
Results. We find that Compton scattering does not change the emergent spectra significantly for low accretion rates or low white dwarf masses. However, it becomes important at high accretion rates and high white dwarf masses. The time-averaged, broad-band X-ray spectrum of intermediate polar V709 Cas obtained by the RXTE and INTEGRAL observatories is fitted using the set of computed spectral models. We obtained the white dwarf mass of and using models with Compton scattering taken into account and without it, respectively.
Key words: stars: binaries: close / stars: novae, cataclysmic variables / stars: white dwarfs / radiative transfer / scattering / stars: atmospheres
© ESO, 2008
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