A&A 435, 191-199 (2005)
DOI: 10.1051/0004-6361:20041283
RXTE broadband X-ray spectra of intermediate polars and white dwarf mass estimates
V. Suleimanov1, 2, 3, M. Revnivtsev2, 4 and H. Ritter21 Kazan State University, Kremlevskaya str. 18, 420008 Kazan, Russia
e-mail: vals@ksu.ru
2 Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei München, Germany
3 Astronomy Division, PO Box 3000, 90014 University of Oulu, Finland
4 Space Research Institute, Russian Academy of Sciences, Profsoyuznaya 84/32, 117810 Moscow, Russia
(Received 13 May 2004 / Accepted 15 December 2004)
Abstract
We present results of an analysis of broadband X-ray
spectra of 14 intermediate polars obtained with the RXTE observatory
(PCA and HEXTE spectrometers, 3-100 keV). For this we have
calculated theoretical models of the structure and the emergent
spectrum of the post-shock region of intermediate polars. By
fitting theoretical model spectra to the observed spectra
we derive estimates for the masses of the white dwarfs.
We compare the resulting masses with masses
obtained by other authors and other methods. The masses obtained by
us are smaller than the masses obtained by using PCA and GINGA
data, and they are in good agreement with the masses
derived from radial velocity studies.
Key words: stars: binaries: close -- stars: binaries: spectroscopic -- X-ray: binaries -- stars: novae, cataclysmic variables
SIMBAD Objects
© ESO 2005

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