Effect of Beam-Plasma Instabilities on Accretion Disk Flares

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dc.creatorKrishan, Vinod
dc.creatorWiita, Paul J.
dc.creatorRamadurai, S.
dc.date2000-02-17
dc.date.accessioned2026-07-07T01:52:22Z
dc.date.available2026-07-07T01:52:22Z
dc.descriptionWe show that a certain class of flare models for variability from accretion disk coronae are subject to beam-plasma instabilities. These instabilities can prevent significant direct acceleration and greatly reduce the variable X-ray emission argued to arise via inverse Compton scattering involving relativistic electrons in beams and soft photons from the disk.
dc.description4 pages, 0 figures, accepted for publication in A&A, uses A&A LaTeX macros
dc.identifierhttps://arxiv.org/abs/astro-ph/0002361
dc.identifierhttp://arxiv.org/abs/astro-ph/0002361
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/601
dc.subjectAstrophysics
dc.titleEffect of Beam-Plasma Instabilities on Accretion Disk Flares
dc.typetext

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