The Orbital Period of the SMC X-ray Pulsar XTE J0055-727

Details The Orbital Period of the SMC X-ray Pulsar XTE J0055-727 The Orbital Period of the SMC X-ray Pulsar XTE J0055-727

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004atel..347....1c&link_type=abstract

The Astronomer's Telegram, #347

Astronomy and Astrophysics

Astronomy

3

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

Scientific paper

Regular monitoring of the Small Magellanic Cloud with the RXTE Proportional Counter Array has revealed a periodicity in the pulsed flux from the 18.4s X-ray pulsar XTE J0055-727, initially found to be active in November/December 2003 (Corbet et al. 2003, ATEL #214). The source was then not detected in weekly monitoring of the SMC until seen to be active on May 21. The source was then next detected on: June 23, July 29, September 1, and October 7.

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