Issue |
A&A
Volume 427, Number 1, November III 2004
|
|
---|---|---|
Page(s) | 293 - 298 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20041214 | |
Published online | 25 October 2004 |
INTEGRAL observations of the peculiar BeX System SAX J2103.5+4545
Institut de Ciència dels Materials, Universitat de València, 46071 Paterna-Valencia, Spain e-mail: pere.blay@uv.es
Received:
3
May
2004
Accepted:
21
July
2004
We present an INTEGRAL data analysis of the X-ray transient SAX
J2103.5+4545 during two outbursts detected in December 2002. The
INTEGRAL coordinates and error circle agree with the position of the
recently proposed optical counterpart. A power-law plus cut-off model
provided a good fit to the 4–150 keV spectrum yielding a photon index of
, a cut-off energy
keV and a folding
energy
keV. The X-ray luminosity in the 4-150
keV energy range was found to be
erg s-1,
assuming a distance of 6.5 kpc. This luminosity, together with the derived
photon index, indicate that the source is in a bright state. A
second pulse period is measured. This value is significantly
smaller than previous measurements, indicating a long-term spin-up
episode.
Key words: accretion, accretion disks / binaries: close / stars: emission-line, Be / stars: pulsars: individuals: SAX J2103.5+4545 / X-rays: binaries / stars: binaries: close
© ESO, 2004
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