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Comparison of theoretical white dwarf cooling timescales (Research Note)

Autor
Salaris, M.; Althaus, L. G.; Garcia-berro, E.
Tipus d'activitat
Article en revista
Revista
Astronomy and astrophysics
Data de publicació
2013-07
Volum
555
Pàgina inicial
1
Pàgina final
8
DOI
https://doi.org/10.1051/0004-6361/201220622 Obrir en finestra nova
Projecte finançador
1728/OC -AR - AGENCIA through the Programa de Modernizacion Tecnologica BID
EUI2009-04170 - ESF EUROCORES Program EuroGENESIS
Enanas blancas: progenitores, evolución, pulsaciones y explosiones
PIP 112-200801-00940
Repositori
http://hdl.handle.net/2117/24247 Obrir en finestra nova
Resum
Context. An accurate assessment of white dwarf cooling times is paramount so that white dwarf cosmochronology of Galactic populations can be put on more solid grounds. This issue is particularly relevant in view of the enhanced observational capabilities provided by the next generation of extremely large telescopes, that will offer more avenues to use white dwarfs as probes of Galactic evolution and test-beds of fundamental physics. Aims. We estimate for the first time the consistency of results...
Citació
Salaris, M.; Althaus, L. G.; Garcia-berro, E. Comparison of theoretical white dwarf cooling timescales (Research Note). "Astronomy and astrophysics", Juliol 2013, vol. 555, p. 1-8.
Paraules clau
stars: evolution, stars: interiors, white dwarfs
Grup de recerca
GAA - Grup d'Astronomia i Astrofísica

Participants

  • Salaris, Maurizio  (autor)
  • Althaus, Leandro G.  (autor)
  • Garcia-berro Montilla, Enrique  (autor)

Arxius