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arXiv · 0908.4335

Infrared identification of 4U1323-619 revisited

Ivan Zolotukhin·Mikhail Revnivtsev·Nikolai Shakura
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Abstract

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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Ivan Zolotukhin, Mikhail Revnivtsev, Nikolai Shakura. 2009-08-29. Infrared identification of 4U1323-619 revisited. https://doi.org/10.1111/j.1745-3933.2009.00768.x

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