Issue |
A&A
Volume 447, Number 3, March I 2006
|
|
---|---|---|
Page(s) | 1027 - 1034 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20053809 | |
Published online | 10 February 2006 |
IGR J16393-4643: a new heavily-obscured X-ray pulsar
1
INTEGRAL Science Data Centre, Chemin d'Ecogia 16, 1290 Versoix, Switzerland e-mail: arash.bodaghee@obs.unige.ch
2
Observatoire de Genève, Chemin des Maillettes 51, 1290 Sauverny, Switzerland
3
School of Physics and Astronomy, University of Southampton, Highfield, Southampton, SO17 1BJ, UK
4
IASF/CNR, Via Gobetti 101, 40129 Bologna, Italy
5
CEA-Saclay, DAPNIA/Service d'Astrophysique, 91191 Gif-sur-Yvette Cedex, France
6
Fédération de recherche APC, Collège de France, 11 place Marcelin Berthelot, 75231 Paris, France
7
IASF/CNR, Via Fosso del Cavaliere 100, 00133 Rome, Italy
Received:
11
July
2005
Accepted:
27
September
2005
An analysis of the high-energy emission from IGR J16393-4643 (=AX J1639.0-4642) is presented using data from INTEGRAL and XMM-Newton. The
source is persistent in the 20–40 keV band at an average flux of erg cm-2 s-1, with variations
in intensity by at least an order of magnitude. A pulse period of 912.0±0.1 s was discovered in the ISGRI and EPIC light curves.
The source spectrum is a strongly-absorbed (
cm-2) power law that features a high-energy cutoff
above 10 keV. Two iron emission lines at 6.4 and 7.1 keV, an iron absorption edge ≳7.1 keV, and a soft excess
emission of
erg cm-2 s-1 between 0.5–2 keV, are detected in the EPIC spectrum.
The shape of the spectrum does not change with the pulse. Its persistence, pulsation, and spectrum place IGR J16393-4643 among
the class of heavily-absorbed HMXBs. The improved position
from EPIC is RA (J2000
and
(
uncertainty) which is compatible with that of 2MASS J16390535-4642137.
Key words: gamma-rays: observations / X-rays: binaries / pulsars: individuals: IGR J16393-4643 / pulsars: individuals: AX J1639.0-4642
© ESO, 2006
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