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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2515
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dc.contributor.authorSahayanathan, S-
dc.contributor.authorMisra, R-
dc.contributor.authorKembhavi, A. K-
dc.contributor.authorKaul, C. L-
dc.date.accessioned2008-06-26T11:45:09Z-
dc.date.available2008-06-26T11:45:09Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 439 - 440en
dc.identifier.urihttp://hdl.handle.net/2248/2515-
dc.description.abstractWe model the observed X-ray/radio knots in Active Galactic Nuclei (AGN) as isotropically expanding spherical plasma clouds fed continously by non-thermal electrons. The time-dependent electron distribution and the emitted photon spectrum are computed using the standard kinetic equation considering synchrotron, adiabatic and inverse Compton cooling processes. We use this model to study the knots of 1136 - 135 and 1150 + 497, recenly observed by Chandra.en
dc.format.extent59184 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..439Sen
dc.subjectActive galactic nucleien
dc.subjectX-raysen
dc.titleAn Expanding Plasma Model for the X-ray/radio knots in KPC-scale Jets of Active Galactic Nucleien
dc.typeArticleen
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