An optical & X-ray study of the counterpart to the SMC X-ray binary pulsar system SXP327

Details An optical & X-ray study of the counterpart to the SMC X-ray binary pulsar system SXP327 An optical & X-ray study of the counterpart to the SMC X-ray binary pulsar system SXP327

2008-03-27

arxiv.org/abs/0803.3941v1

Astronomy and Astrophysics

Astrophysics

5 pages Accepted for publication in MNRAS

Scientific paper

10.1111/j.1365-2966.2008.13257.x

Optical and X-ray observations are presented here of a newly reported X-ray transient system in the Small Magellanic Cloud. The data reveal many previously unknown X-ray detections of this system and clear evidence for a 49.995d binary period. In addition, the optical photometry show recurring outburst features at the binary period which may well be indicative of the neutron star interacting with a circumstellar disk around a Be star.

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