Modelling Oscillations in GRS 1915+105 Jet Emission

dc.creatorCollins, Ross S.
dc.creatorKaiser, Christian R.
dc.creatorCox, Simon J.
dc.date2002-07-18
dc.date.accessioned2026-07-07T02:04:22Z
dc.date.available2026-07-07T02:04:22Z
dc.descriptionWe have studied time variability in the flux from the flat spectrum synchrotron radiation of the Blandford & Konigl (1979) model for relativistic, conical jets. The resulting model has been applied to the flux variation of the flat spectrum of GRS 1915+105 observed by Fender & Pooley (2000). This comparison has highlighted a fundamental problem of the Blandford & Konigl (1979) model in that it requires unphysically large electron densities to explain the flux levels observed from the flat spectrum of GRS 1915+105.
dc.description3 pages, 1 figure, to appear in the "Proceedings of the 4th Microquasar Workshop", 2002, eds. Durouchoux, Fuchs & Rodriguez, published by the Center for Space Physics: Kolkata. For original poster and animations see http://www.astro.soton.ac.uk/~rsc/ckc02.html
dc.identifierhttps://arxiv.org/abs/astro-ph/0207384
dc.identifierhttp://arxiv.org/abs/astro-ph/0207384
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4725
dc.subjectAstrophysics
dc.titleModelling Oscillations in GRS 1915+105 Jet Emission
dc.typetext

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