2004/09/27 by P. A. Evans, Phil Evans, Evans, P. A. +3
Mathematics · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gas Dynamics and Kinetic Theory #Quantum and Classical Electrodynamics #Relativity and Gravitational Theory #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0409638
6 pages, 6 figures. To appear in "The astrophysics of cataclysmic variables and related objects", ASP Conf. Ser. eds J.M. Hameury & J.P. Lasota
openalex publication_date 2004/09/27 · arxiv created 2004/11/23 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
XMM-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.