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 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006xmm..prop..109m&link_type=abstract

XMM-Newton Proposal ID #05028401

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Igr J14536-5522, Xmm-Newton Proposal 05028401

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, or an equally rare soft IP. We plan to study this object using optical, XMM-Newton, and Swift/BAT data.

Affiliated with

Also associated with

No associations

Rating

The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Hard X-ray Bright Magnetic CV IGR J14536-5522=Swift J1453.4-5524 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1022590