High energy emission from IGR J16320-4751

Simple item page
dc.creatorFoschini, L.
dc.creatorTomsick, J. A.
dc.creatorRodriguez, J.
dc.creatorWalter, R.
dc.creatorGoldwurm, A.
dc.creatorCorbel, S.
dc.creatorKaaret, P.
dc.date2004-03-19
dc.date2004-08-27
dc.date.accessioned2026-07-07T02:12:41Z
dc.date.available2026-07-07T02:12:41Z
dc.descriptionIGR J16320-4751 was re-discovered by IBIS/ISGRI on board INTEGRAL in early February 2003 during the observation of the black hole candidate 4U 1630-47 (PI Tomsick). This source, already observed by ASCA and BeppoSAX, belongs to the class of heavily absorbed objects (N_H > 10^23 cm^-2) that populate some arms of the Galaxy. Soon after the rediscovery by IBIS/ISGRI, the source was observed by XMM-Newton: the arcsec position found with XMM allowed ones to find the most likely infrared counterpart. We present here the reanalysis of the high energy emission from IGR J16320-4751 detected by IBIS/ISGRI, including the spectral and temporal characteristics. We also present a reanalysis of the XMM-Newton and optical/IR data.
dc.description8 pages, 6 figures. Revised after referee's comments. Accepted for publication on the Proceedings of the V INTEGRAL Workshop, Munich 16-20 February 2004 (ESA SP-552)
dc.identifierhttps://arxiv.org/abs/astro-ph/0403479
dc.identifierhttp://arxiv.org/abs/astro-ph/0403479
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7540
dc.subjectAstrophysics
dc.titleHigh energy emission from IGR J16320-4751
dc.typetext

Files

Collections

arXiv