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INTEGRAL Broadband X-ray spectrum of the intermediate polar V709 Cas

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arxiv astro-ph/0509489 v1 submitted 2005-09-16 astro-ph

classification astro-ph
keywords v709x-rayenergyintegralintermediatepolarpost-shockspectrum

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We present the hard X-ray time-averaged spectrum of the intermediate polar V709 Cas observed with INTEGRAL. We performed the observation using data from the IBIS/ISGRI instrument in the 20-100 keV energy band and from JEM-X at lower energy (5-20 keV). Using different multi-temperature and density X-ray post-shock models we measured a improved post-shock temperature of ~40 keV and estimated the V709 Cas mass to be 0.82(+0.12/-0.25} Msun. We compare the resulting spectral parameters with previously reported BeppoSAX and RXTE observations.

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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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