The disc-jet connection in GRS 1915+105

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dc.creatorKlein-Wolt, M.
dc.creatorFender, R. P.
dc.creatorPooley, G. G.
dc.creatorBelloni, T.
dc.creatorMigliari, S.
dc.creatorMorgan, E. H.
dc.creatorvan der Klis, M.
dc.date2000-11-01
dc.date.accessioned2026-07-07T01:56:20Z
dc.date.available2026-07-07T01:56:20Z
dc.descriptionWe have compared simultaneous Ryle Telescope (RT) radio and Rossi X-Ray Timing Explorer (RXTE) X-ray observations of the galactic microquasar GRS 1915+105. We find that radio emission, and therefore also the radio jet, requires the presence of long (~100s), hard dips in the X-ray light curve which seem to have a one-to-one relation with the radio events: each hard dip produces a new radio "flare". We discuss the characteristic features of the connection between the hard X-ray states and the radio emission.
dc.description2 pages, 1 figure, to be published in `Proceedings of the Third Microquasar Workshop: Granada Workshop on galactic relativistic jet sources', Eds A. J.Castro-Tirado, J. Greiner and J. M. Paredes, Astrophysics and Space Science, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0011011
dc.identifierhttp://arxiv.org/abs/astro-ph/0011011
dc.identifierAstrophys.Space Sci. 276 (2001) 291-292
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1963
dc.subjectAstrophysics
dc.titleThe disc-jet connection in GRS 1915+105
dc.typetext

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