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arXiv · 0910.0954

Hard X-ray properties of magnetic cataclysmic variables

S. Scaringi·A. J. Bird·A. J. Norton·C. Knigge·A. B. Hill·D. J. Clark·A. J. Dean·V. A. McBride·E. J. Barlow·L. Bassani·A. Bazzano·M. Fiocchi·R. Landi
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Abstract

Hard X-ray surveys have proven remarkably efficient in detecting intermediate polars and asynchronous polars, two of the rarest type of cataclysmic variable (CV). Here we present a global study of hard X-ray selected intermediate polars and asynchronous polars, focusing particularly on the link between hard X-ray properties and spin/orbital periods. To this end, we first construct a new sample of these objects by cross-correlating candidate sources detected in INTEGRAL/IBIS observations against catalogues of known CVs. We find 23 cataclysmic variable matches, and also present an additional 9 (of which 3 are definite) likely magnetic cataclysmic variables (mCVs) identified by others through optical follow-ups of IBIS detections. We also include in our analysis hard X-ray observations from Swift/BAT and SUZAKU/HXD in order to make our study more complete. We find that most hard X-ray detected mCVs have P_{spin}/P_{orb}<0.1 above the period gap. In this respect we also point out the very low number of detected systems in any band between P_{spin}/P_{orb}=0.3 and P_{spin}/P_{orb}=1 and the apparent peak of the P_{spin}/P_{orb} distribution at about 0.1. The observational features of the P_{spin} - P_{orb} plane are discussed in the context of mCV evolution scenarios. We also present for the first time evidence for correlations between hard X-ray spectral hardness and P_{spin}, P_{orb} and P_{spin}/P_{orb}. An attempt to explain the observed correlations is made in the context of mCV evolution and accretion footprint geometries on the white dwarf surface.

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S. Scaringi, A. J. Bird, A. J. Norton, C. Knigge, A. B. Hill, D. J. Clark, A. J. Dean, V. A. McBride, E. J. Barlow, L. Bassani, A. Bazzano, M. Fiocchi, R. Landi. 2009-10-06. Hard X-ray properties of magnetic cataclysmic variables. https://doi.org/10.1111/j.1365-2966.2009.15826.x

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