2007A&A...467..249S


C.D.S. - SIMBAD4 rel 1.7 - 2019.09.23CEST18:10:39

2007A&A...467..249S - Astronomy and Astrophysics, volume 467, 249-257 (2007/5-3)

IGR J18483-0311: an accreting X-ray pulsar observed by INTEGRAL.

SGUERA V., HILL A.B., BIRD A.J., DEAN A.J., BAZZANO A., UBERTINI P., MASETTI N., LANDI R., MALIZIA A., CLARK D.J. and MOLINA M.

Abstract (from CDS):

IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23-28 April 2003. To detect new outbursts from IGR J18483-0311 using INTEGRAL and archival Swift XRT observations and finally to characterize the nature of this source using the optical/near-infrared (NIR) information available through catalogue searches. We performed an analysis of light curves and spectra of INTEGRAL and archival Swift XRT data as well as of optical/NIR catalogues. We report on 5 newly discovered outbursts from IGR J18483-0311 detected by INTEGRAL. For two of them it was possible to constrain a duration of the order of a few days. The strongest outburst reached a peak flux of ∼120mCrab (20-100keV); its broad band JEM-X/ISGRI spectrum (3-50keV) is best fitted by an absorbed cutoff power law with Γ=1.4±0.3, cutoff energy of 22+7.5–4.5keV and NH=9+5–4x1022cm–2. Timing analysis of INTEGRAL data allowed us to identify periodicities of 18.52 days and 21.0526 seconds which are likely the orbital period of the system and the spin period of the X-ray pulsar respectively. Swift XRT observations of IGR J18483-0311 provided a very accurate source position which strongly indicates a highly reddened star in the USNO-B1.0 and 2MASS catalogues as its possible optical/NIR counterpart. The X-ray spectral shape, the periods of 18.52-days and 21.0526s, the high intrinsic absorption, the location in the direction of the Scutum spiral arm and the highly reddened optical object as possible counterpart, all favour the hypothesis that IGR J18483-0311 is a HMXB with a neutron star as compact companion. The system is most likely a Be X-ray binary, but a Supergiant Fast X-ray Transient nature can not be entirely excluded.

Abstract Copyright:

Journal keyword(s): gamma rays: observations - X-rays: binaries - X-rays: bursts - X-rays: general - X-rays: individual: IGR J18483-0311 - X-rays: binaries

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2019
#notes
1 NAME Crux-Scutum Spiral Arm reg 12 30 -60.0           ~ 263 0
2 [KRL2007b] 129 Psr 13 01 58.7203639191 -63 58 08.830169485           O9V/B1III 50 0
3 NAME Gal Center reg 17 45 40.04 -29 00 28.1           ~ 10931 0
4 IGR J18483-0311 HXB 18 48 17.2064881183 -03 10 16.876608322 23.702 25.162 21.884 17.888 15.88 B0.5Ia 108 0
5 NAME Sgr Arm PoG 19 00 -30.0           ~ 494 1
6 NAME Scutum Spiral Arm PoG ~ ~           ~ 255 0

    Equat.    Gal    SGal    Ecl

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2019.09.23-18:10:39

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