Original title:
Comparison of relativistic iron line models
Translated title:
Porovnání modelů relativistické čáry železa
Authors:
Svoboda, Jiří ; Dovčiak, Michal ; Goosmann, René ; Karas, Vladimír Document type: Papers Conference/Event: Week of Doctoral Students 2008, Praha (CZ), 2008-06-03 / 2008-06-06
Year:
2008
Language:
eng Abstract:
[eng][cze] The analysis of the broad iron line profile in the X-ray spectra of active galactic nuclei and black hole X-ray binaries allows us to constrain the spin parameter of the black hole. We compare the constraints on the spin value for two X-ray sources, MCG-6-30-15 and GX 339-4, with a broad iron line using present relativistic line models in XSPEC - LAOR and KYRLINE.Analýza profilu široké čáry železa v rentgenových spektrech aktivních galaxií a mikrokvasarů nám umožňuje určit spin černé díry. Porovnávame výsledky pro dva rentgenové zdroje, MCG-6-30-15 a GX 339-4, se širokou čárou železa pomocí současných modelů relativistické čáry v programu XSPEC - LAOR a KYRLINE.
Keywords:
accretion; accretion disks; black holes Project no.: CEZ:AV0Z10030501 (CEP), ESA-PECS Project No. 98040 Funding provider: EU Host item entry: WDS'08 Proceedings of Contributed Papers, ISBN 978-80-7378-024-1
Institution: Astronomical Institute AS ČR
(web)
Document availability information: Fulltext is available at the institute of the Academy of Sciences. Original record: http://hdl.handle.net/11104/0170211