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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2436
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dc.contributor.authorChattopadhyay, I-
dc.contributor.authorChakrabarti, S. K-
dc.date.accessioned2008-06-16T12:09:57Z-
dc.date.available2008-06-16T12:09:57Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 313 - 316en
dc.identifier.urihttp://hdl.handle.net/2248/2436-
dc.description.abstractWe study effects of radiation momentum deposition on jets and outflows from the disks and show that if disks are perturbed, jets could have propagating shock waves which may accelerate particles to observed slopes.en
dc.format.extent300315 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..313Cen
dc.subjectAstrophysical Jetsen
dc.subjectShocksen
dc.subjectSynchrotron Radiationen
dc.titleShocks in winds from accretion discs and the formation of high energy particlesen
dc.typeArticleen
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