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Warm absorber and truncated accretion disc in IRAS 05078+1626
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SYSNO ASEP 0345820 Document Type J - Journal Article R&D Document Type Journal Article Subsidiary J Článek ve WOS Title Warm absorber and truncated accretion disc in IRAS 05078+1626 Author(s) Svoboda, Jiří (ASU-R) RID, ORCID
Guainazzi, M. (IT)
Karas, Vladimír (ASU-R) RID, ORCIDNumber of authors 3 Source Title Astronomy & Astrophysics. - : EDP Sciences - ISSN 0004-6361
Roč. 512, Mar-Apr (2010), A62/1-A62/8Number of pages 8 s. Language eng - English Country FR - France Keywords galaxies: active ; galaxies: Seyfert ; galaxies: individual: IRAS 05078+1626 Subject RIV BN - Astronomy, Celestial Mechanics, Astrophysics R&D Projects GD205/09/H033 GA ČR - Czech Science Foundation (CSF) GA205/07/0052 GA ČR - Czech Science Foundation (CSF) CEZ AV0Z10030501 - ASU-R (2005-2011) UT WOS 000276245500029 DOI 10.1051/0004-6361/200913659 Annotation We investigate the central environment of a Seyfert 1.5 galaxy IRAS 05078+1626 with the EPIC and RGS instruments onboard XMM-Newton. Our study represents the first X-ray spectroscopic measurement of this galaxy. The spectrum unveils some of the standard ingredients in Seyfert galaxies, such as a power law primary continuum, modified by reflection from the accretion disc and by the effect of complex, multi-phase obscuration. However, data constrains the accretion disc, if present, not to extend closer than to 60 gravitational radii from the black hole. Workplace Astronomical Institute Contact Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326 Year of Publishing 2011
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