Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2542
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dc.contributor.authorGangadhara, R. T-
dc.contributor.authorKrishan, V-
dc.date.accessioned2008-06-30T06:49:58Z-
dc.date.available2008-06-30T06:49:58Z-
dc.date.issued1992-05-
dc.identifier.citationMNRAS, Vol. 256, No. 1, pp. 111 - 120en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2542-
dc.description.abstractThere are three ways in which an electromagnetic wave can undergo scattering in a plasma: (1) when the scattering of radiation occurs by a single electron, it is called Compton Scattering; (2) if it occurs by a longitudinal electron plasma mode, it is called Stimulated Raman Scattering (SRS); and (3) if it occurs by a highly damped electron plasma mode, it is called Stimulated Compton Scattering (SCS). The nonthermal continuum of quasars is believed to be produced through the combined action of synchrotron and inverse Compton processes, which are essentially single-particle processes. The role of SRS and SCS in the generation of continuum radiation from these compact objects is investigated. It is shown as an example that the complete spectrum of 3C 273 can be reproduced by suitably combining SCS and SRS. The differential contributions of SCS and SRS under different values of the plasma parameters are also calculated.en
dc.format.extent1490274 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishingen
dc.relation.urihttp://adsabs.harvard.edu/abs/1992MNRAS.256..111Gen
dc.subjectCompton effecten
dc.subjectCosmic plasmaen
dc.subjectElectron scatteringen
dc.subjectQuasarsen
dc.subjectRaman spectraen
dc.subjectAngular distributionen
dc.subjectAstronomical spectroscopyen
dc.subjectComputational astrophysicsen
dc.subjectLorentz transformationsen
dc.subjectWave scatteringen
dc.titleThe role of Compton and Raman scattering in the quasar continuumen
dc.typeArticleen
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