Orbital properties of an unusually low-mass sdB star in a close binary system with a white dwarf
We have used 605 days of photometric data from the Kepler spacecraft to study KIC 6614501, a close binary system with an orbital period of 0.15749747(25) days (3.779939 h), that consists of a low-mass subdwarf B (sdB) star and a white dwarf (WD). As seen in many other similar systems, the gravitatio...
Guardado en:
| Autor principal: | Althaus, Leandro Gabriel |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2012
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84638 |
| Aporte de: |
Ejemplares similares
-
Close-In Substellar Companions and the Formation of sdB-Type Close Binary Stars
por: Zhu, Lei, et al.
Publicado: (2015) -
Evolution of low-mass close binary systems with a neutron star: Its dependence with the initial neutron star mass
por: De Vito, María Alejandra, et al.
Publicado: (2010) -
The evolution of low-mass, close binary systems with a neutron star component: a detailed grid
por: De Vito, María Alejandra, et al.
Publicado: (2012) -
A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR cae
por: Qian, S. B., et al.
Publicado: (2012) -
The formation of helium white dwarfs in close binary systems – II
por: Benvenuto, Omar Gustavo, et al.
Publicado: (2005)