Fast Infrared Sub-Flares From GRS 1915+105

dc.creatorRothstein, David M.
dc.creatorEikenberry, Stephen S.
dc.date2002-08-02
dc.date.accessioned2026-07-07T02:04:33Z
dc.date.available2026-07-07T02:04:33Z
dc.descriptionWe report the discovery of fast (~ 100 sec) 2.2 micron flares from the microquasar GRS 1915+105, which are superimposed on longer (~ 30 min), brighter flares corresponding to episodes of jet formation. The number and strength of the sub-flares in each bright flare varies, and does not seem to correlate in any obvious way with the underlying light curve or with changes in the X-ray emission. However, the fact that these sub-flares only occur in tandem with the larger flares indicates that they might be related to the jet ejection process.
dc.description4 pages, 2 figures; to appear in Proceedings of the 4th Microquasar Workshop, eds. Ph Durouchoux, Y. Fuchs and J. Rodriguez, published by the Center for Space Physics: Kolkata
dc.identifierhttps://arxiv.org/abs/astro-ph/0208068
dc.identifierhttp://arxiv.org/abs/astro-ph/0208068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4800
dc.subjectAstrophysics
dc.titleFast Infrared Sub-Flares From GRS 1915+105
dc.typetext

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