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Title:
Exploring the Hard and Soft X-ray Emission of Magnetic Cataclysmic Variables
Authors:
de Martino, D.; Anzolin, G.; Bonnet-Bidaud, J.-M.; Falanga, M.; Matt, G.; Mouchet, M.; Mukai, K.; Masetti, N.
Affiliation:
AA(INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, Naples 80131, Italy), AB(INAF-Osservatorio Astronomico di Capodimonte, Via Moiariello 16, Naples 80131, Italy), AC(Service d'Astrophysique, Saclay Gif-Sur-Yvette, France), AD(Service d'Astrophysique, Saclay Gif-Sur-Yvette, France), AE(Dipartimento di Fisica, Universitá Roma Tre, Roma, Italy), AF(Laboratoire APC, Université Paris 7, Paris), AG(CRESST and X-Ray Astrophysics Laboratory, NASA/GSFC, Greenbelt, USA), AH(INAF-IASF Bologna, Italy)
Publication:
SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium. AIP Conference Proceedings, Volume 1126, pp. 210-212 (2009). (AIPC Homepage)
Publication Date:
05/2009
Origin:
AIP
PACS Keywords:
X-ray sources; X-ray bursts, Infall, accretion, and accretion disks, X-ray, Spectroscopy and spectrophotometry
DOI:
10.1063/1.3149415
Bibliographic Code:
2009AIPC.1126..210D

Abstract

A non-negligible fraction of galactic hard (>20 keV) X-ray sources were identified as CVs of the magnetic Intermediate Polar type in INTEGRAL, SWIFT and RXTE surveys, that suggests a still hidden but potentially important population of faint hard X-ray sources. Simbol-X has the unique potential to simultaneously characterize their variable and complex soft and hard X-ray emission thus allowing to understand their putative role in galactic populations of X-ray sources.
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