XMM-Newton observation of the highly magnetized accreting pulsar Swift J045106.8−694803: evidence of a hot thermal excess

Several persistent, low-luminosity (L X ∼ 1034 erg s−1), long-spin-period (P > 100 s) high-mass X-ray binaries have been reported with blackbody components with temperatures >1 keV. These hot thermal excesses have correspondingly small emitting regions (2 keV) and soft (

Saved in:
Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2013-12, Vol.436 (3), p.2054-2062
Main Authors: Bartlett, E. S., Coe, M. J., Ho, W. C. G.
Format: Article
Language:English
Citations: Items that this one cites
Items that cite this one
Online Access:Request full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Several persistent, low-luminosity (L X ∼ 1034 erg s−1), long-spin-period (P > 100 s) high-mass X-ray binaries have been reported with blackbody components with temperatures >1 keV. These hot thermal excesses have correspondingly small emitting regions (2 keV) and soft (
ISSN:0035-8711
1365-2966
DOI:10.1093/mnras/stt1711