The Quiet HMXB Candidates HD 14633 and HD 15137

Details The Quiet HMXB Candidates HD 14633 and HD 15137 The Quiet HMXB Candidates HD 14633 and HD 15137

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007xmm..prop..112m&link_type=abstract

XMM-Newton Proposal ID #05538102

Computer Science

Stars, White Dwarfs, Solar System, Hd 14633, Hd 15137, Xmm-Newton Proposal Id #05538102

Scientific paper

The runaway O-type binaries HD 14633 and HD 15137 were likely ejected from the cluster of their birth by supernovae explosions in close binaries. Neither star is a known X-ray source, but they likely contain neutron stars and may be weak stellar wind accretion systems. Hence the two binaries have been classified as "quiet HMXBs". We propose observations with XMM-Newton that will detect the hard power-law spectrum from accreting or quiescent neutron star companions and reveal their evolutionary history.

Affiliated with

Also associated with

No associations

Rating

The Quiet HMXB Candidates HD 14633 and HD 15137 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 Quiet HMXB Candidates HD 14633 and HD 15137, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Quiet HMXB Candidates HD 14633 and HD 15137 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-955275