Period study of RS Sagittarii

New times of minimum for the eclipsing binary RS Sgr were determined. These minima were added with previous photoelectric, photographic, and visual estimates. A weighted linear and parabolic least squares fit was performed with all minima. The result of this fit is that the period is constant betwee...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: De Laurenti, M.A., Cerruti, M.A.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Astronomía
Galaxia
rs sgr
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142176
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata

Ejemplares similares

Ejemplares similares