New SMC X-ray Pulsar in 37 d binary and showing large amplitude super-orbital variations.

Details New SMC X-ray Pulsar in 37 d binary and showing large amplitude super-orbital variations. New SMC X-ray Pulsar in 37 d binary and showing large amplitude super-orbital variations.

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3154....1r&link_type=abstract

The Astronomer's Telegram, #3154

Astronomy and Astrophysics

Astronomy

Optical, X-Ray, Binary, Star, Transient, Variables, Pulsar

Scientific paper

We have detected a new X-ray pulsar in the direction of the SMC using archival Chandra data (Observation ID 2758) which we designate SXP707. This observation (time interval 2002-08-27 04:04:23 - 18:15:24; useful exposure time 49.45 ks) shows a very significant detection of an X-ray source at RA= 01:04:28.7; Dec.= -72:31:34 (J2000) with an observed flux of 3.2 x 10-13 ergs/cm2/s and luminosity of 1.4 x 1035 ergs/s (0.2 - 10.0 keV, assuming d= 60 kpc).

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