Abstract
The evolution of white dwarfs is essentially a cooling process that lasts for ~ 10 Gyr. Since the study of white dwarfs allows to obtain information about the age of the Galaxy (Winget et al. 1987, García-Berro et al. 1988, Hernanz et al. 1994), it is important to identify all the sources of energy as well as the mechanisms that control its outflow.KeywordsWhite DwarfGlobular ClusterSolid CoreCrystallization FrontCataclysmic VariableThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.
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