The effect of <SUP>22</SUP>Ne diffusion in the evolution and pulsational properties of white dwarfs with solar metallicity progenitors
Because of the large neutron excess of 22Ne, sedimentation of this isotope occurs rapidly in the interior of white dwarfs. This process releases an additional amount of energy, thus delaying the cooling times of the white dwarf. This influences the ages of different stellar populations derived using...
Guardado en:
| Autores principales: | Camisassa, María Eugenia, Althaus, Leandro Gabriel, Córsico, Alejandro Hugo, Vinyoles, N., Serenelli, Aldo Marcelo, Isern, J., Miller Bertolami, Marcelo Miguel, García Berro, E. |
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| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2016
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/86799 |
| Aporte de: |
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