Eclipse mapping of the stream and disk flickering components in V2051 Oph

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dc.creatorBaptista, R.
dc.creatorBortoletto, A.
dc.date2004-10-07
dc.date.accessioned2026-07-07T02:14:58Z
dc.date.available2026-07-07T02:14:58Z
dc.descriptionWe report on the investigation of the spatial distribution of the flickering sources in the dwarf nova V2051 Oph with eclipse mapping techniques. Low-frequency flickering originates in the gas stream and is related to the mass transfer process, whereas high-frequency flickering arises in the accretion disk and is probably connected to magneto-hydrodynamic turbulence.
dc.description2 pages, no figures. To appear in The astrophysics of cataclysmic variables and related objects, ASP Conf. Ser., eds. J.M. Hameury and J.P. Lasota
dc.identifierhttps://arxiv.org/abs/astro-ph/0410216
dc.identifierhttp://arxiv.org/abs/astro-ph/0410216
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8338
dc.subjectAstrophysics
dc.titleEclipse mapping of the stream and disk flickering components in V2051 Oph
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