Photometric Period of XTE J0053-724 (SXP46.6 = 1WGA J0053.8-7226)

Details Photometric Period of XTE J0053-724 (SXP46.6 = 1WGA J0053.8-7226) Photometric Period of XTE J0053-724 (SXP46.6 = 1WGA J0053.8-7226)

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atel.1316....1s&link_type=abstract

The Astronomer's Telegram, #1316

Astronomy and Astrophysics

Astronomy

1

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

Scientific paper

We have analyzed 7 years of OGLE-III photometry for the SMC X- ray pulsar XTE J0053-724 (SXP46.6). The optical counterpart is star 30 of field SMC108.8 in the OGLE-III database. It corresponds to the Be star marked as Star B on the finding chart of Buckley et al. (2001, MNRAS, 320, 281). M. Coe has pointed out on his web site (www.astro.soton.ac.uk/~mjc/smc/ Finders/sxp46.6.jpg) that this star is most consistent with the Chandra X-ray position (00:53:53.8; -72:26:35).

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