Confirmation of the optical identification and binary period in IGR J05007-7047

Details Confirmation of the optical identification and binary period in IGR J05007-7047 Confirmation of the optical identification and binary period in IGR J05007-7047

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010atel.2597....1c&link_type=abstract

The Astronomer's Telegram, #2597

Astronomy and Astrophysics

Astronomy

1

Optical, X-Ray, Binaries, Neutron Stars

Scientific paper

The optical counterpart to IGR J05007-7047 can be found in the OGLE III database as source named LMC130.4 19472. Timing analysis of eight years of monitoring of this system in the I-band reveals a clear period at 30.80 ± 0.03d, together with the beat period associated with the annual sampling cycle. This confirms the period seen in the X-ray band by La Parola et al in ATEL #2594 and the optical counterpart identified by Halpern in ATEL #572.

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