Title of article :
Phase resolved study of the CRSF in MX 0656-072 Original Research Article
Author/Authors :
V.A. McBride، نويسنده , , W. Coburn، نويسنده , , M.J. Coe، نويسنده , , P. Kretschmar، نويسنده , , I. Kreykenbohm، نويسنده , , R.E. Rothschild، نويسنده , , R. Staubert، نويسنده , , J. Wilms، نويسنده ,
Issue Information :
دوهفته نامه با شماره پیاپی سال 2006
Abstract :
MXB 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 160.4 s and a cyclotron resonance scattering feature in the spectrum at ∼32 keV. This paper presents pulse profile analysis and phase-resolved X-ray spectroscopy of RXTE observations during this outburst.
Keywords :
X-rays , stars , magnetic fields , Stars , Stars , pulsars
Journal title :
Advances in Space Research
Journal title :
Advances in Space Research
