Reflection Spectra from Photoionized Accretion Discs

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dc.creatorBallantyne, D. R.
dc.creatorRoss, R. R.
dc.creatorFabian, A. C.
dc.date2002-04-16
dc.date.accessioned2026-07-07T02:03:25Z
dc.date.available2026-07-07T02:03:25Z
dc.descriptionWe review recent progress on the modeling and use of reflection spectra from irradiated and ionized accretion discs. On the computational side, calculations of reflection spectra from discs with non-uniform density structure have shown that thermal instabilities can effect the predictions. Ionized reflection spectra have been used effectively in fitting data of Narrow-Line Seyfert 1 galaxies, and have placed constraints on the strength and shape of soft X-ray emission lines.
dc.description4 pages, 4 figs. To appear in 'X-ray Spectroscopy of AGN with Chandra and XMM-Newton', held in Garching, December 3-6, 2001, eds. Th. Boller et al
dc.identifierhttps://arxiv.org/abs/astro-ph/0204260
dc.identifierhttp://arxiv.org/abs/astro-ph/0204260
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4378
dc.subjectAstrophysics
dc.titleReflection Spectra from Photoionized Accretion Discs
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