New orbital period, plus clarification on pulse periods, for X-ray pulsars in the SMC

Details New orbital period, plus clarification on pulse periods, for X-ray pulsars in the SMC New orbital period, plus clarification on pulse periods, for X-ray pulsars in the SMC

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..674....1g&link_type=abstract

The Astronomer's Telegram, #674

Astronomy and Astrophysics

Astronomy

4

X-Ray, Binaries, Neutron Stars, Pulsars, Transients

Scientific paper

The Small Magellanic Cloud pulsar SXP169 (XTE J0054-720, RX J0052.9-7158) was discovered by Lochner et al. (1997, IAUC #6814). SXP165 was reported by Corbet et al. (2004, AIP Conf. Proc. 714, 337). Using data from the weekly monitoring campaign of the SMC carried out with the RXTE Proportional Counter Array, a search was carried out for pulsations around a central period of 167.35s, and encompassing both pulsars.

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