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...

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Detalles Bibliográficos
Autores principales: De Laurenti, M.A., Cerruti, M.A.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1988
Materias:
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/142176
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id I19-R120-10915-142176
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxia
rs sgr
spellingShingle Astronomía
Galaxia
rs sgr
De Laurenti, M.A.
Cerruti, M.A.
Period study of RS Sagittarii
topic_facet Astronomía
Galaxia
rs sgr
description 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 between the errors of the parabolic coefficient (∼1.0x10⁻¹⁰). The "history" of the system is about 14000 cycles (1895-1985).
format Articulo
Comunicacion
author De Laurenti, M.A.
Cerruti, M.A.
author_facet De Laurenti, M.A.
Cerruti, M.A.
author_sort De Laurenti, M.A.
title Period study of RS Sagittarii
title_short Period study of RS Sagittarii
title_full Period study of RS Sagittarii
title_fullStr Period study of RS Sagittarii
title_full_unstemmed Period study of RS Sagittarii
title_sort period study of rs sagittarii
publishDate 1988
url http://sedici.unlp.edu.ar/handle/10915/142176
work_keys_str_mv AT delaurentima periodstudyofrssagittarii
AT cerrutima periodstudyofrssagittarii
bdutipo_str Repositorios
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