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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3054
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dc.contributor.authorKrishan, V-
dc.contributor.authorWiita, P. J-
dc.contributor.authorRamadurai, S-
dc.date.accessioned2008-08-08T05:50:19Z-
dc.date.available2008-08-08T05:50:19Z-
dc.date.issued2000-04-
dc.identifier.citationAstronomy and Astrophysics, Vol. 356, No.1, pp. 373 - 376en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3054-
dc.description.abstractWe 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.en
dc.format.extent99317 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000A%26A...356..373Ken
dc.subjectAccretionen
dc.subjectAccretion disksen
dc.subjectPlasmasen
dc.subjectSun: flaresen
dc.subjectGalaxies: activeen
dc.subjectX-Rays: generalen
dc.titleEffect of beam-plasma instabilities on accretion disk flaresen
dc.typeArticleen
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