Los cúmulos globulares más ricos en estrellas variables

Autores
Wilkens, Herbert
Año de publicación
1963
Idioma
español castellano
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The publication of the figures of 37 globular clusters (only 2 figures in this Bulletin) characterized by possessing variable stars in them -while the variables of the surrounding field appear more or less separated from them- has the object of proving that the apparent diameter of these clusters were estimated correctly with the help of these variables. These apparent diameters were the base of a previous theoretical investigation of the author on "Luminosity and diameter of globular clusters I", La Plata, Serie Circular Nº 16. The paper will be published in the same "Serie Circular".
Asociación Argentina de Astronomía
Materia
Ciencias Astronómicas
Cúmulos globulares
diiámetros
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/90963

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network_name_str SEDICI (UNLP)
spelling Los cúmulos globulares más ricos en estrellas variablesThe richest globular clusters in variable starsWilkens, HerbertCiencias AstronómicasCúmulos globularesdiiámetrosThe publication of the figures of 37 globular clusters (only 2 figures in this Bulletin) characterized by possessing variable stars in them -while the variables of the surrounding field appear more or less separated from them- has the object of proving that the apparent diameter of these clusters were estimated correctly with the help of these variables. These apparent diameters were the base of a previous theoretical investigation of the author on "Luminosity and diameter of globular clusters I", La Plata, Serie Circular Nº 16. The paper will be published in the same "Serie Circular".Asociación Argentina de Astronomía1963info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf45-48http://sedici.unlp.edu.ar/handle/10915/90963spainfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-09-03T10:51:21Zoai:sedici.unlp.edu.ar:10915/90963Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-09-03 10:51:21.61SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Los cúmulos globulares más ricos en estrellas variables
The richest globular clusters in variable stars
title Los cúmulos globulares más ricos en estrellas variables
spellingShingle Los cúmulos globulares más ricos en estrellas variables
Wilkens, Herbert
Ciencias Astronómicas
Cúmulos globulares
diiámetros
title_short Los cúmulos globulares más ricos en estrellas variables
title_full Los cúmulos globulares más ricos en estrellas variables
title_fullStr Los cúmulos globulares más ricos en estrellas variables
title_full_unstemmed Los cúmulos globulares más ricos en estrellas variables
title_sort Los cúmulos globulares más ricos en estrellas variables
dc.creator.none.fl_str_mv Wilkens, Herbert
author Wilkens, Herbert
author_facet Wilkens, Herbert
author_role author
dc.subject.none.fl_str_mv Ciencias Astronómicas
Cúmulos globulares
diiámetros
topic Ciencias Astronómicas
Cúmulos globulares
diiámetros
dc.description.none.fl_txt_mv The publication of the figures of 37 globular clusters (only 2 figures in this Bulletin) characterized by possessing variable stars in them -while the variables of the surrounding field appear more or less separated from them- has the object of proving that the apparent diameter of these clusters were estimated correctly with the help of these variables. These apparent diameters were the base of a previous theoretical investigation of the author on "Luminosity and diameter of globular clusters I", La Plata, Serie Circular Nº 16. The paper will be published in the same "Serie Circular".
Asociación Argentina de Astronomía
description The publication of the figures of 37 globular clusters (only 2 figures in this Bulletin) characterized by possessing variable stars in them -while the variables of the surrounding field appear more or less separated from them- has the object of proving that the apparent diameter of these clusters were estimated correctly with the help of these variables. These apparent diameters were the base of a previous theoretical investigation of the author on "Luminosity and diameter of globular clusters I", La Plata, Serie Circular Nº 16. The paper will be published in the same "Serie Circular".
publishDate 1963
dc.date.none.fl_str_mv 1963
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://sedici.unlp.edu.ar/handle/10915/90963
url http://sedici.unlp.edu.ar/handle/10915/90963
dc.language.none.fl_str_mv spa
language spa
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by-nc-sa/4.0/
Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
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45-48
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
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