Spectral and temporal properties of the X-ray pulsar SMC X-1 at hard X-rays

The binary X-ray pulsar SMC X- 1 has been observed at hard X-rays with the High Energy X-Ray Experiment (HEXE) on nine occasions between Nov. 1987 and March 1989. A thin thermal bremsstrahlung fit to the phase averaged spectrum yields a plasma temperature (14.4 +/- 1.3) keV and a luminosity above (1...

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Bibliographic Details
Published in:Astronomy and astrophysics (Berlin) 1993-02, Vol.268 (1), p.116-122
Main Authors: Kunz, M., Gruber, D. E., Kendziorra, E ., Kretschmar, P., Maisack, M., Mony, B., Staubert, R., Doebereiner, S., Englhauser, J., Pietsch, W.
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Earth, ocean, space
Exact sciences and technology
Late stages of stellar evolution (including black holes)
Neutron stars
Stars
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Summary:The binary X-ray pulsar SMC X- 1 has been observed at hard X-rays with the High Energy X-Ray Experiment (HEXE) on nine occasions between Nov. 1987 and March 1989. A thin thermal bremsstrahlung fit to the phase averaged spectrum yields a plasma temperature (14.4 +/- 1.3) keV and a luminosity above (1.1 +/- 0.1) x 10 exp 38 erg/s in the 20-80 keV band. Pulse period values have been established for three observations, confirming the remarkably stable spin-up trend of SMC X-1. In one of the three observations the pulse profile was seen to deviate from a dominant double pulsation, while at the same time the pulsed fraction was unusually large. For one observation we determined for the first time the pulsed fraction in narrow energy bands. It increases with photon energy from about 20 percent up to over 60 percent in the energy range from 20 to 80 keV.
ISSN:0004-6361
1432-0746