Infrared identification of 4U1323-619 revisited

Details Infrared identification of 4U1323-619 revisited Infrared identification of 4U1323-619 revisited

2009-08-29

arxiv.org/abs/0908.4335v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 pages, 1 table, 1 figure, accepted to MNRAS Letters

Scientific paper

We re-examine the infrared counterpart of the dipping low-mass x-ray binary 4U1323-619. New X-ray data available from the XMM and Chandra observatories combined with archival IR observations from the ESO 3.6m New Technology Telescope allow us to define a new possible counterpart. We present here its photometric properties and compare them with a simple analytical model of an accretion disc illuminated by the hot central corona known to be present in the binary system.

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