The Orbital Period of the X-ray Pulsar XTE SMC144s

Details The Orbital Period of the X-ray Pulsar XTE SMC144s The Orbital Period of the X-ray Pulsar XTE SMC144s

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003atel..209....1c&link_type=abstract

The Astronomer's Telegram, #209

Astronomy and Astrophysics

Astronomy

2

X-Ray, Binaries, Neutron Stars, Transients

Scientific paper

We have detected three additional outbursts from the 144s pulse period transient X-ray pulsar in the direction of the Small Magellanic Cloud with the RXTE Proportional Counter Array since the outburst that was reported in ATEL #163. We have continued to monitor the SMC since that time with observations made at intervals of approximately one week. The first outburst from "XTE SMC144s" was detected on 2003 May 19 and subsequent outbursts were detected on July 21, September 22, and November 18.

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