Accretion instabilities and jet formation in GRS 1915+105

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dc.creatorMirabel, I. F.
dc.creatorDhawan, V.
dc.creatorChaty, S.
dc.creatorRodriguez, L. F.
dc.creatorMarti, J.
dc.creatorRobinson, C. R.
dc.creatorSwank, J.
dc.creatorGeballe, T.
dc.date1997-11-10
dc.date1997-11-14
dc.date.accessioned2026-07-07T02:24:59Z
dc.date.available2026-07-07T02:24:59Z
dc.descriptionWe report simultaneous observations in the X-ray, infrared, and radio wavelengths of the galactic superluminal source GRS 1915+105. During episodes of rapid disappearance and follow up replenishment of the inner accretion disk evidenced by the X-ray oscillating flux, we observe the ejection of relativistic plasma clouds in the form of synchrotron flares at infrared and radio wavelengths. The expelled clouds contain very energetic particles with Lorentz factors of about 1000, or more. These ejections can be viewed as small-scale analogs of the more massive ejecta with relativistic bulk motions that have been previously observed in GRS 1915+105.
dc.description4 pages, LaTeX, special macro espf.sty, with 3 color figures, to appear in Astronomy and Astrophysics Letters replaced version, with only minor changes
dc.identifierhttps://arxiv.org/abs/astro-ph/9711097
dc.identifierhttp://arxiv.org/abs/astro-ph/9711097
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11769
dc.subjectAstrophysics
dc.titleAccretion instabilities and jet formation in GRS 1915+105
dc.typetext

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