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.


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    Titel :

    Phase resolved study of the CRSF in MX 0656-072


    Beteiligte:
    McBride, V.A. (Autor:in) / Coburn, W. (Autor:in) / Coe, M.J. (Autor:in) / Kretschmar, P. (Autor:in) / Kreykenbohm, I. (Autor:in) / Rothschild, R.E. (Autor:in) / Staubert, R. (Autor:in) / Wilms, J. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 38 , 12 ; 2768-2770


    Erscheinungsdatum :

    2006-02-22


    Format / Umfang :

    3 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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