Two extreme contact binary systems in the nearest globular cluster M4
We present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson-Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the s...
Guardado en:
| Autores principales: | Liu, L., Qian, S. B., Fernández Lajús, Eduardo |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2011
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83953 |
| Aporte de: |
Ejemplares similares
-
V752 Cen – a triple-lined spectroscopic contact binary with sudden and continuous period changes
por: Zhou, Xiaojuan, et al.
Publicado: (2019) -
Evidence of a massive black hole companion in the massive eclipsing binary V Puppis
por: Qian, S. B., et al.
Publicado: (2008) -
Evolutionary states of the two shortest period O-type overcontact binaries V382 Cyg and TU Mus
por: Qian, S. B., et al.
Publicado: (2007) -
Confirmation and revision on the orbital period change of the possible type Ia supernova progenitor V617 Sagittarii
por: Shi, Guang, et al.
Publicado: (2014) -
RW Doradus: a solar-type shallow contact binary with a new orbital period investigation
por: Sarotsakulchai, Thawicharat, et al.
Publicado: (2019)