Phase resolved study of the CRSF in MX 0656-072
McBride, V. A., Coburn, W., Coe, M. J., Kretschmar, P., Kreykenbohm, I., Rothschild, R. E., Staubert, R. and Wilms, J.. (2006) Phase resolved study of the CRSF in MX 0656-072. ADVANCES IN SPACE RESEARCH, 38 (12). pp. 2768-2770. ISSN 0273-1177Full text not available from this repository.
Official URL: http://dx.doi.org/10.1016/j.asr.2006.02.081
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.
|Item Type:||Journal Article|
|Subjects:||T Technology > TL Motor vehicles. Aeronautics. Astronautics
Q Science > QB Astronomy
Q Science > QE Geology
Q Science > QC Physics
|Journal or Publication Title:||ADVANCES IN SPACE RESEARCH|
|Publisher:||ELSEVIER SCI LTD|
|Number of Pages:||3|
|Page Range:||pp. 2768-2770|
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