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• W2994920993 abstract "The Eclipse Mapping Method is an indirect imaging technique that transforms the shape of the eclipse light curve into a map of the surface brightness distribution of the occulted regions. Three decades of application of this technique to the investigation of the structure, the spectrum and the time evolution of accretion discs around white dwarfs in cataclysmic variables have enriched our understanding of these accretion devices with a wealth of details such as (but not limited to) moving heating/cooling waves during outbursts in dwarf novae , tidally-induced spiral shocks of emitting gas with sub-Keplerian velocities, elliptical precessing discs associated to superhumps , and measurements of the radial run of the disc viscosity through the mapping of the disc flickering sources. This chapter reviews the principles of the method, discusses its performance, limitations, useful error propagation procedures, as well as highlights a selection of applications aimed at showing the possible scientific problems that have been and may be addresses with it." @default.
• W2994920993 created "2019-12-26" @default.
• W2994920993 creator A5012757780 @default.
• W2994920993 date "2016-01-01" @default.
• W2994920993 modified "2023-09-30" @default.
• W2994920993 title "Eclipse Mapping: Astrotomography of Accretion Discs" @default.
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• W2994920993 doi "https://doi.org/10.1007/978-3-319-39739-9_9" @default.
• W2994920993 hasPublicationYear "2016" @default.
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