Binary period in Optical counterpart to XMMU J004723.7-731226 (SXP 264)

Details Binary period in Optical counterpart to XMMU J004723.7-731226 (SXP 264) Binary period in Optical counterpart to XMMU J004723.7-731226 (SXP 264)

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..405....1e&link_type=abstract

The Astronomer's Telegram, #405

Astronomy and Astrophysics

Astronomy

3

X-Ray, Binaries, Pulsars, Transients

Scientific paper

A probable binary period has been detected in the optical counterpart to the X-ray source XMMU J004723.7-731226 = RXJ0047.3-7312 = AXJ0047.3-7312= SXP 264 in the Small Magellanic Cloud. This source has been identified with the emission line star [MA93]172 and is coincident with Optical Gravitational Lensing (OGLE) objects 116979 (Phase II) and 45007 (Phase III) (Udalski et al., 1998). We find an optical period of 48.8 +/- 0.6 days in the OGLE data.

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