Formation and evolution of a 0.242 <i>M</i><SUB>⊙</SUB> solar masses helium white dwarfs in presence of element diffusion
Conventional wisdom indicates that a millisecond pulsar is recycled during the mass transfer stage in a binary system. Usually, the companion to the pulsar is a low-mass white dwarf. If zero ages are set at the end of mass transfer, the ages of both objects should be the same. Available models chara...
Guardado en:
| Autores principales: | Althaus, Leandro Gabriel, Serenelli, Aldo Marcelo, Benvenuto, Omar Gustavo |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2001
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/2056 http://iopscience.iop.org/article/10.1086/321414/meta |
| Aporte de: |
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