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Paper: Eclipse Mapping of the Stream and Disk Flickering Components in V2051 Oph
Volume: 330, The Astrophysics of Cataclysmic Variables and Related Objects
Page: 367
Authors: Baptista, R.; Bortoletto, A.
Abstract: We 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.
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