| HAL : in2p3-00356684, version 1 |
| arXiv : 0901.3351 |
| Code Bibliographique ADS : 2009A&A...498...61T |
| DOI : 10.1051/0004-6361/200810944 |
| Fiche détaillée | Récupérer au format |
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| Astronomy and Astrophysics 498 (2009) 61-66 |
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| 3C 33: another case of photoionized soft X-ray emission in radio galaxies |
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| E. Torresi1, 2P. Grandi2M. GuainazziG.G.C. Palumbo1G. Ponti3S. Bianchi4 |
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| (2009) |
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| All the observations available in the Chandra and XMM-Newton archives have been used to investigate the X-ray spectral properties of 3C 33. In this paper is presented a complete X-ray analysis of the nuclear emission of this narrow line radio galaxy. The broad band spectrum of 3C 33 is complex. The hard part resembles that of Seyfert 2 galaxies, with a heavily obscured nuclear continuum (N_H~10^23 cm^-2) and a prominent Fe Kalpha line. This represents the nuclear radiation directly observed in transmission through a cold circumnuclear gas. On the other hand an unabsorbed continuum plus emission lines seem to fit well the soft part of the spectrum (0.5-2 keV) suggesting that the jet does not significantly contribute to the X-ray emission. We discuss the possible collisional or photoionized origin of the gas that emits the soft X-ray lines. Our results, strengthened by optical spectroscopy favor the photoionization scenario. |
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| APC - AHE |
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| Thème(s) | : | Physique/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique Planète et Univers/Astrophysique/Phénomènes cosmiques de haute energie Physique/Astrophysique/Phénomènes cosmiques de haute energie |
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| galaxies: active – X-rays: galaxies – X-rays: individuals: 3C 33 |
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| Lien vers le texte intégral : |
| in2p3-00356684, version 1 | |
| http://hal.in2p3.fr/in2p3-00356684 | |
| oai:hal.in2p3.fr:in2p3-00356684 | |
| Contributeur : Simone Lantz | |
| Soumis le : Jeudi 29 Janvier 2009, 11:58:59 | |
| Dernière modification le : Lundi 25 Juin 2012, 15:10:01 | |