Binary period in Optical counterpart to CXOU J005455.6-724510 = RXJ0054.9-7245 = AX J0054.8-7244 = SXP504

Details Binary period in Optical counterpart to CXOU J005455.6-724510 = RXJ0054.9-7245 = AX J0054.8-7244 = SXP504 Binary period in Optical counterpart to CXOU J005455.6-724510 = RXJ0054.9-7245 = AX J0054.8-7244 = SXP504

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005atel..426....1e&link_type=abstract

The Astronomer's Telegram, #426

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 CXOU J005455.6-724510 = RX J0054.9-7245 = AXJ0054.8-7244 = SXP504 in the Small Magellanic Cloud. This source was detected by Chandra on 04 Jul 2002 (MJD 52459) and first reported in ATEL#217. It was subsequently observed by XMM-Newton on 18 Dec 2003 (MJD 52991) (ATEL#219). The source is coincident with the Optical Gravitational Lensing (OGLE) object numbered 47103 (in Phase II) and 36877 (in Phase III) (Udalski et al., 1998).

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