AbstractMXB 0656-072 is an accreting X-ray pulsar with a Be star companion, showing notable emission in Hα. In October 2003 this system exhibited a large and extended X-ray outburst. RXTE observations during this outburst indicated a pulse period of 160.4s and a cyclotron resonance scattering feature in the spectrum at ∼32keV. This paper presents pulse profile analysis and phase-resolved X-ray spectroscopy of RXTE observations during this outburst.
Phase resolved study of the CRSF in MX 0656-072
Advances in Space Research ; 38 , 12 ; 2768-2770
2006-02-22
3 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
X-rays , stars , Stars , magnetic fields , pulsars
Phase resolved study of the CRSF in MX 0656-072
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