A brief review of long-term X-ray and optical variability in radio-quiet AGN

dc.creatorUttley, Philip
dc.creatorMcHardy, Ian M.
dc.date2004-02-17
dc.date.accessioned2026-07-07T10:47:47Z
dc.date.available2026-07-07T10:47:47Z
dc.descriptionLong-time-scale X-ray and optical variability is a key characteristic of AGN. Here, we summarise our current understanding of the X-ray and optical continuum variability of radio-quiet AGN and the relation between the two bands. We demonstrate the strong connection between the X-ray variability properties of AGN and the variability of stellar-mass black hole candidates on much shorter time-scales, and discuss the implications of this result for the origins of the variability. The relationship between optical and X-ray variability is complex, with some AGN showing strong X-ray/optical correlations while others show no obvious correlation. We suggest a possible explanation for this variety of behaviour.
dc.description8 pages, invited contribution to the conference 'Stellar mass, Intermediate-mass and Supermassive black holes', October 28-31 2003, Kyoto, Japan (proceedings to be published in Progress of Theoretical Physics)
dc.identifierhttps://arxiv.org/abs/astro-ph/0402407
dc.identifierhttp://arxiv.org/abs/astro-ph/0402407
dc.identifierProg.Theor.Phys.Suppl.155:170-177,2004
dc.identifierdoi:10.1143/PTPS.155.170
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183656
dc.subjectAstrophysics
dc.titleA brief review of long-term X-ray and optical variability in radio-quiet AGN
dc.typetext

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