Understanding the evolution of close binary systems with radio pulsars
We calculate the evolution of close binary systems (CBSs) formed by a neutron star (behaving as a radio pulsar) and a normal donor star, which evolve either to a helium white dwarf (HeWD) or to ultra-short orbital period systems. We consider X-ray irradiation feedback and evaporation due to radio pu...
Guardado en:
| Autores principales: | Benvenuto, Omar Gustavo, De Vito, María Alejandra, Horvath, J. E. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2014
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84865 |
| Aporte de: |
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