Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259

Details Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259 Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2252....1b&link_type=abstract

The Astronomer's Telegram, #2252

Astronomy and Astrophysics

Astronomy

X-Ray, Gamma Ray, Binaries, Neutron Stars, Pulsars

Scientific paper

Re-analysis of a Swift/XRT ToO observation of IGR J01572-7259 in the Magellanic Bridge (=IGR J015712-7259, c.f. Coe et al., 2008, ATel #1882) has enabled us to establish the first soft X-ray spectrum for this 11.6-s X-ray pulsar and suspected high-mass X-ray binary. Observation-ID 00031313001 was taken on December 20, 2008, for an effective exposure time of 1950 s. The 0.5-7 keV spectrum was fit with a power law including a photoelectric absorption component that assumed either Solar abundances or those described by Wilms et al., 2000.

Affiliated with

Also associated with

No associations

Rating

Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259 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 Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Swift/XRT spectrum of the accreting X-ray pulsar IGR J01572-7259 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1355888