New models for the evolution of post-asymptotic giant branch stars and central stars of planetary nebulae

Context. The post-asymptotic giant branch (AGB) phase is arguably one of the least understood phases of the evolution of low- and intermediate- mass stars. The two grids of models presently available are based on outdated micro- and macrophysics and do not agree with each other. Studies of the centr...

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Detalles Bibliográficos
Autor principal:	Miller Bertolami, Marcelo Miguel
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2016
Materias:	Ciencias Astronómicas Planetary nebulae: general Stars: AGB and post-AGB Stars: evolution Stars: low-mass
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85962
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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