The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524

Details The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524 The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop...97m&link_type=abstract

XMM-Newton Proposal ID #05530501

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Igr J14536-5522, Xmm-Newton Proposal Id #05530501

Scientific paper

Cataclysmic variables (CVs) are an important class of X-ray emitting objects, including the hard X-ray (>10 keV) regime that INTEGRAL and Swift have begun to explore. Many CVs detected above 10 keV so far are well known objects, but some are little known or previously unnoticed objects. Many detections are standard intermediate polars (IPs), the hard X-ray brightest subclass of CVs; however, some appear to be more exotic. Here we propose a 25 ks observation of a previously unknown CV, IGR J14536-5522=Swift JJ1453.4-5524. It is likely to be a rare, hard X-ray bright polar. We plan to study this object using optical, XMM-Newton, and Swift/BAT data.

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