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The white dwarf population within 40 pc of the Sun

Autor
Torres, S.; Garcia-berro, E.
Tipus d'activitat
Article en revista
Revista
Astronomy & astrophysics
Data de publicació
2016-04-01
Volum
588
DOI
https://doi.org/10.1051/0004-6361/201528059 Obrir en finestra nova
Projecte finançador
Simulaciones multidimensionales de novas y supernovas
Repositori
http://hdl.handle.net/2117/101451 Obrir en finestra nova
URL
http://www.aanda.org/articles/aa/abs/2016/04/aa28059-15/aa28059-15.html Obrir en finestra nova
Resum
© 2016 ESO. Context. The white dwarf luminosity function is an important tool to understand the properties of the solar neighborhood, like its star formation history, and its age. Aims. 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. Methods. We use a state-of-the-art population synthesis code based on Monte Carlo techniques, which incorporates the most recent ...
Citació
Torres, S., Garcia-berro, E. The white dwarf population within 40 pc of the Sun. "Astronomy & astrophysics", 1 Abril 2016, vol. 588.
Paraules clau
Galaxy: evolution, Stars: luminosity function, White dwarfs, mass function
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants

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