What can XMM-Newton tell us about the spin periods of Intermediate Polars?

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dc.creatorEvans, P. A.
dc.creatorHellier, Coel
dc.date2004-09-27
dc.date2004-11-23
dc.date.accessioned2026-07-07T02:14:45Z
dc.date.available2026-07-07T02:14:45Z
dc.descriptionXMM-Newton's unprecedented combination of spectral resolution and high throughput allows us to perform the best phase-resolved X-ray analysis of intermediate polars to date. The Optical Monitor gives optical/UV photometry simultaneously with the X-ray data. We present a comprehensive study of X-ray spin pulses in IPs, giving spin-pulses and hardness ratios for every IP looked at with XMM-Newton to date.
dc.description6 pages, 6 figures. To appear in "The astrophysics of cataclysmic variables and related objects", ASP Conf. Ser. eds J.M. Hameury & J.P. Lasota
dc.identifierhttps://arxiv.org/abs/astro-ph/0409638
dc.identifierhttp://arxiv.org/abs/astro-ph/0409638
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8241
dc.subjectAstrophysics
dc.titleWhat can XMM-Newton tell us about the spin periods of Intermediate Polars?
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