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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2255
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dc.contributor.authorYadav, J. S-
dc.date.accessioned2008-04-23T11:29:52Z-
dc.date.available2008-04-23T11:29:52Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 271 - 276en
dc.identifier.urihttp://hdl.handle.net/2248/2255-
dc.description.abstractOne of the Galactic Black-hole Candidates GRS 1915+105 has shown spectacular variability on various time scales in X-ray, Infrared (IR) and Radio wavelengths and has been extensively studied in multiwavelengths during last few years. This X-ray transient source has earned the name "microquasar" as it is known to emit superluminal relativistic radio jets. Since microquasars are much smaller, closer and show faster variability than the extragalactic systems (quasars and other active galactic nuclei (AGNs), they are supposed to be potential "laboratories" for the study of black hole accretion relativistic jet systems. We summarise here some of the exciting multiwavelength studies of this source and discuss the progress made in understanding the accretion disk - jet connection.en
dc.format.extent536379 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..271Yen
dc.subjectAccretionen
dc.subjectBlack hole binariesen
dc.subjectX-raysen
dc.subjectRadioen
dc.subjectJetsen
dc.titleMultiwavelength studies of galactic black-hole candidatesen
dc.typeArticleen
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