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On the fate of extremely low metallicity stars

Autor
Gil Pons, P.; Gutierrez, J.; Garcia-berro, E.; Althaus, L. G.
Tipus d'activitat
Article en revista
Revista
AIP Conference proceedings
Data de publicació
2008
Volum
1001
Pàgina inicial
71
Pàgina final
78
DOI
10.1063/1.2916992
Repositori
http://hdl.handle.net/2117/17386 Obrir en finestra nova
URL
http://proceedings.aip.org/resource/2/apcpcs/1001/1/71_1?isAuthorized=no Obrir en finestra nova
Resum
We have computed and analyzed the evolution of intermediate-mass stars of metallicity Z = 10−5 from the main sequence until the early stages of the TP-(S)AGB phase. In order to check the influence of mixing we have performed our calculations using two different evolutionary codes, EVOLVE — which does not include diffusion but allows for overshooting— and LPCODE, which includes diffusion and overshooting “à-la-Herwig”. Important differences appear during the TP– AGB phase, as the cal...
Citació
Gil Pons, P. [et al.]. On the fate of extremely low metallicity stars. "AIP Conference proceedings", 2008, vol. 1001, p. 71-78.
Grup de recerca
DF - Dinàmica de Fluids: formació d'estructures i aplicacions geofísiques
GAA - Grup d'Astronomia i Astrofísica

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