arXiv · astro-ph/0411547
Discovery of X-ray pulsations from IGR J16320-4751 = AX J1631.9-4752
Abstract
We report a discovery of strong modulations of the X-ray flux detected from IGR J16320-4751 = AX J1631.9-4752 with a period of P~1300 sec. We reanalyzed the data of an XMM-Newton ToO performed soon after the discovery of the source by INTEGRAL and found the modulation at a period of P=1309+/-40 sec with a high significance. Modulations of the source flux with two possible periods of ~1300 and ~1500 sec were identified in the ASCA archival data. It is very likely that the modulation can be interpreted as X-ray pulsations, favouring a pulsar as the compact object in IGR/AX J16320-4752. Thus for the moment this source became the fourth source from a new class of highly absorbed binary systems for which the pulsations are observed.
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A. Lutovinov, J. Rodriguez, M. Revnivtsev, P. Shtykovskiy. 2005-02-23. Discovery of X-ray pulsations from IGR J16320-4751 = AX J1631.9-4752. https://doi.org/10.1051/0004-6361%3A200500092
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