Issue |
A&A
Volume 448, Number 3, March IV 2006
|
|
---|---|---|
Page(s) | 873 - 880 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361:20053744 | |
Published online | 03 March 2006 |
An INTEGRAL hard X-ray survey of the Large Magellanic Cloud
1
INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica, via Bassini 15, 20133 Milano, Italy e-mail: diego@iasf-milano.inaf.it
2
Dipartimento di Fisica - Università degli Studi di Milano, via Celoria 16, 20133 Milano, Italy
3
INAF - Osservatorio Astronomico di Brera, via E. Bianchi 46, 23807 Merate, Italy
Received:
1
July
2005
Accepted:
27
October
2005
Two observation campaigns in 2003 and 2004 with the
INTEGRAL satellite have provided the first sensitive survey of the
Large Magellanic Cloud with an imaging instrument in the hard
X-ray range (15 keV–10 MeV). The high energy flux and long-term variability of the black hole
candidate LMC X–1 was measured for the first time without contamination
by the nearby (~25′) young pulsar PSR B0540–69.
We studied the accreting pulsar LMC X–4 by constraining the size of the
hard X-ray emitting region (≤3 1010 cm) from analysis
of its eclipses and by measuring its spin period (13.497 ± 0.005 s) in the 20–40 keV band.
As it was in a soft state during the first observation and possibly
in an extremely low state in the second one, LMC X–3 was not detected.
Thanks to the large field of view of the IBIS instrument, we could also study
other sources falling serendipitously in the
observed sky region around the LMC: the Galactic low mass X-ray
binary EXO 0748–676, the accreting pulsar SMC X–1 in the Small Magellanic
Cloud, and the Active Galactic Nucleus IRAS 04575–7537. In addition we discovered
five new hard X-ray sources, two of which most likely belong to the LMC.
Key words: gamma-rays: observations / pulsars: individual: PSR B0540–69 / X-rays: binaries / X-rays: galaxies / Magellanic Clouds
© ESO, 2006
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