Evolutionary states of the two shortest period O-type overcontact binaries V382 Cyg and TU Mus
Up to now, V382 Cyg and TU Mus are the only two discovered O-type overcontact binary stars with periods less than two days (P = 1.8855 and 1.3873 d). Both systems contain a visual companion. New eclipse times and analyses of orbital period variations of the two systems are presented. It is discovere...
Guardado en:
| Autores principales: | Qian, S. B., Yuan, J. Z., Liu, L., He, J. J., Fernández Lajús, Eduardo Eusebio, Kreiner, J. Z. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2007
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93868 https://academic.oup.com/mnras/article/380/4/1599/1062514 https://ri.conicet.gov.ar/handle/11336/41984 |
| Aporte de: |
Ejemplares similares
-
A charge-coupled device photometric study of south hemispheric contact binary ae phoenicis
por: He, J. J., et al.
Publicado: (2009) -
RW Doradus: a solar-type shallow contact binary with a new orbital period investigation
por: Sarotsakulchai, Thawicharat, et al.
Publicado: (2019) -
Differential corrections analysis of the UBVRI observations of AG phoenicis
por: Cerruti, M.A. -
Differential corrections analysis of the UBV observations of LT Pavonis
por: Cerruti, M.A. -
Differential corrections analysis of the UBVRI observations of AG phoenicis
Publicado: (2000)