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| HAL : in2p3-00712230, version 1 |
| arXiv : 1202.3594 |
| Code Bibliographique ADS : 2012MmSAI..83..578M |
| Fiche détaillée |  Récupérer au format |
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| Workshop on the golden age of cataclysmic variables and related objects, Palermo : Italie (2012) |
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| The X-ray emission of magnetic cataclysmic variables in the XMM-Newton era |
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| M. Mouchet1, 2J.M. Bonnet-Bidaud3D. de Martino |
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| (02/2013) |
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| We review the X-ray spectral properties of magnetic cataclysmic binaries derived from observations obtained during the last decade with the large X-ray observatories XMM-Newton, Chandra and Suzaku. We focus on the signatures of the different accretion modes which are predicted according to the values of the main physical parameters (magnetic field, local accretion rate and white dwarf mass). The observed large diversity of spectral behaviors indicates a wide range of parameter values in both intermediate polars and polars, in line with a possible evolutionary link between both classes. |
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| 1 : | APC - AstroParticule et Cosmologie |
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| 2 : | LUTH - Laboratoire Univers et Théories |
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| 3 : | IRFU - Institut de Recherches sur les lois Fondamentales de l'Univers (ex DAPNIA) |
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| APC - Cosmologie et gravitation |
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| Thème(s) | : | Physique/Astrophysique/Phénomènes cosmiques de haute energie Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie |
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| Lien vers le texte intégral : |
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| http://fr.arXiv.org/abs/1202.3594 |
| in2p3-00712230, version 1 | |
| http://hal.in2p3.fr/in2p3-00712230 | |
| oai:hal.in2p3.fr:in2p3-00712230 | |
| Contributeur : M. Mouchet | |
| Soumis le : Mardi 26 Juin 2012, 16:39:00 | |
| Dernière modification le : Mercredi 15 Mai 2013, 16:36:47 | |
