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

Several persistent, low-luminosity (LX ~ 10^sup 34^ erg s^sup -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 (

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2013-12, Vol.436 (3), p.2054
Main Authors: Bartlett, E S, Coe, M J, Ho, W CG
Format: Article
Language:English
Subjects:
Astronomy
Luminosity
Pulsars
Spectrum analysis
Temperature
Online Access:Get full text
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Description
Summary:Several persistent, low-luminosity (LX ~ 10^sup 34^ erg s^sup -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