Issue |
A&A
Volume 444, Number 2, December III 2005
|
|
---|---|---|
Page(s) | 561 - 564 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361:20054002 | |
Published online | 25 November 2005 |
INTEGRAL broadband X-ray spectrum of the intermediate polar V709 Cassiopeiae
1
CEA Saclay, DSM/DAPNIA/Service d'Astrophysique (CNRS FRE 2591), 91191 Gif-sur-Yvette, France e-mail: mfalanga@cea.fr
2
Unité mixte de recherche Astroparticule et Cosmologie, 11 place Berthelot, 75005 Paris, France
3
Kazan State University, Kremlevskaya str. 18, 420008 Kazan, Russia
4
Astronomy Division, PO Box 3000, 90014 University of Oulu, Finland
5
Kazan Branch of Isaac Newton Institute, Santiago, Chile
Received:
6
August
2005
Accepted:
14
September
2005
We present the hard X-ray time-averaged spectrum of the
intermediate polar V709 Cas observed with INTEGRAL. We performed the
observation using data from the IBIS/ISGRI instrument in the 20–100 keV
energy band and from JEM-X at lower energy (5–20 keV).
Using different multi-temperature and density X-ray post-shock models
we measured an improved post-shock temperature of ~40 keV and
estimated the V709 Cas mass to be 0.82
. We
compare the resulting spectral parameters with previously reported BeppoSAX
and RXTE observations.
Key words: binaries: general / stars: individual: V709 Cas / X–rays: stars
© ESO, 2005
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