volume 13, issue S334, P374-375 2017
DOI: 10.1017/s174392131700730x
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Santiago Torres, Florian Nutten, Georgy Skorobogatov, Enrique García-Berro

Abstract: AbstractWhite dwarfs are natural cosmochronometers, and this allows us to use them to study relevant properties of the Galaxy, such as its age or its star formation rate history. Here we present a population synthesis study of the white dwarf population within 40 pc from the Sun, and compare the results of this study with the properties of the observed sample. We use a state-of-the-art population synthesis code based on Monte Carlo techniques that incorporates the most recent and reliable white dwarf cooling s…

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