Correlated msec X-ray and optical emission from XTE J1118+480

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dc.creatorKanbach, G.
dc.creatorStraubmeier, C.
dc.creatorSpruit, H. C.
dc.creatorBelloni, T.
dc.date2001-08-11
dc.date2001-10-15
dc.date.accessioned2026-07-07T01:59:38Z
dc.date.available2026-07-07T01:59:38Z
dc.descriptionWe report on fast (msec) simultaneous observations in X-rays and optical light of the black hole candidate XTE J1118+480, showing correlation on time scales from 20msec to several seconds. The shape of the correlation is not easily explained with existing models. We suggest that is is caused by optical cyclosynchrotron emission in a dense, relatively slow outflow from the inner regions of the accretion.
dc.descriptionRevised version as accepted by Nature. Please do not discuss with popular press before publication date
dc.identifierhttps://arxiv.org/abs/astro-ph/0108199
dc.identifierhttp://arxiv.org/abs/astro-ph/0108199
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3193
dc.subjectAstrophysics
dc.titleCorrelated msec X-ray and optical emission from XTE J1118+480
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