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- W2029631328 abstract "MXB 0656-072 is an accreting X-ray pulsar with a Be star companion, showing notable emission in Hoc. 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 similar to 32 keV. This paper presents pulse profile analysis and phase-resolved X-ray spectroscopy of RXTE observations during this outburst. (c) 2006 COSPAR. Published by Elsevier Ltd. All rights reserved." @default.
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- W2029631328 date "2006-01-01" @default.
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- W2029631328 title "Phase resolved study of the CRSF in MX 0656-072" @default.
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- W2029631328 doi "https://doi.org/10.1016/j.asr.2006.02.081" @default.
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