Lithium production in the merging of white dwarf stars
The origin of R Coronae Borealis stars has been elusive for over 200 years. Currently, two theories for their formation have been presented. These are the final flash scenario, in which a dying asymptotic giant branch star throws off its atmosphere to reveal the hydrogen poor, heavily processed mate...
Guardado en:
| Autores principales: | Longland, R., Lorén Aguilar, P., José, J., García Berro, E., Althaus, Leandro Gabriel |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83974 |
| Aporte de: |
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