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RXTE broadband X-ray spectra of intermediate polars and white dwarf mass estimates

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arxiv astro-ph/0405236 v1 pith:OG46H7VI submitted 2004-05-12 astro-ph

V. Suleimanov (1 , 2) , M. Revnivtsev (2 , 3) , H. Ritter (2)((1) Kazan State University , Kazan , Russia , (2) MPA
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Garching Germany (3) IKI Moscow Russia)
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We present results of an analysis of broadband spectra of 14 intermediate polars obtained with the RXTE observatory (PCA and HEXTE spectrometers, 3-100 keV). By means of our calculations of the structure and the emergent spectrum of the post-shock region of intermediate polars we fitted the observed spectra and obtained estimates of the white dwarf masses. The estimated masses are compared with masses obtained by other authors.

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Cited by 1 Pith paper

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  1. Long-term Optical Photometry of V709 Cas Using TESS : Refined Periods and Accretion Geometry

    astro-ph.SR 2025-07 conditional novelty 5.0 of 10

    The white dwarf binary V709 Cas shows refined periods (5.3329 h, 312.7478 s, 317.9267 s) and time-variable accretion geometry consistent with a two-pole disc-overflow accretor.

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