Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121

Autores
Baume, Gustavo Luis; Noël, N. E. D.; Costa, E.; Carraro, Giovanni; Méndez, R. A.; Pedreros, M. H.
Año de publicación
2008
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present observations for three star clusters, Kron 11, Kron 63 and NGC 121, in the Small Magellanic Cloud. We have studied their structure and derived their fundamental parameters by means of their luminosity functions, their colour magnitude diagrams and the Padova suite of isochrones. NGC 121 is a well-studied object, for which we confirm previous evidence about its old age and low-metal content, and have found that it is an undergoing mass segregation. Kron 11 and Kron 63 are poorly populated clusters which had never been studied so far. Kron 11 is several gigayears younger than NGC 121, while Kron 63 is basically a very young star aggregate. Both clusters are immersed in dense stellar fields which share the same population properties, suggesting that in their cases, cluster ages are consistent with typical ages of field stars.
Fil: Baume, Gustavo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Noël, N. E. D.. Instituto de Astrofísica de Canarias; España
Fil: Costa, E.. Universidad de Chile; Chile
Fil: Carraro, Giovanni. European Southern Observatory; Chile
Fil: Méndez, R. A.. Universidad de Chile; Chile
Fil: Pedreros, M. H.. Universidad de Taracapà; Chile
Materia
Galaxies
Stars
Kron 11 (estrella)
Kron 63 (estrella)
NGC 121 (estrella)
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/43218

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network_name_str CONICET Digital (CONICET)
spelling Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121Baume, Gustavo LuisNoël, N. E. D.Costa, E.Carraro, GiovanniMéndez, R. A.Pedreros, M. H.GalaxiesStarsKron 11 (estrella)Kron 63 (estrella)NGC 121 (estrella)https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present observations for three star clusters, Kron 11, Kron 63 and NGC 121, in the Small Magellanic Cloud. We have studied their structure and derived their fundamental parameters by means of their luminosity functions, their colour magnitude diagrams and the Padova suite of isochrones. NGC 121 is a well-studied object, for which we confirm previous evidence about its old age and low-metal content, and have found that it is an undergoing mass segregation. Kron 11 and Kron 63 are poorly populated clusters which had never been studied so far. Kron 11 is several gigayears younger than NGC 121, while Kron 63 is basically a very young star aggregate. Both clusters are immersed in dense stellar fields which share the same population properties, suggesting that in their cases, cluster ages are consistent with typical ages of field stars.Fil: Baume, Gustavo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; ArgentinaFil: Noël, N. E. D.. Instituto de Astrofísica de Canarias; EspañaFil: Costa, E.. Universidad de Chile; ChileFil: Carraro, Giovanni. European Southern Observatory; ChileFil: Méndez, R. A.. Universidad de Chile; ChileFil: Pedreros, M. H.. Universidad de Taracapà; ChileWiley Blackwell Publishing, Inc2008-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/43218Baume, Gustavo Luis; Noël, N. E. D.; Costa, E.; Carraro, Giovanni; Méndez, R. A.; et al.; Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 390; 12-2008; 1683-16900035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13860.xinfo:eu-repo/semantics/altIdentifier/url/https://onlinelibrary.wiley.com/toc/13652966/390/4info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:29:42Zoai:ri.conicet.gov.ar:11336/43218instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:29:43.134CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
title Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
spellingShingle Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
Baume, Gustavo Luis
Galaxies
Stars
Kron 11 (estrella)
Kron 63 (estrella)
NGC 121 (estrella)
title_short Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
title_full Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
title_fullStr Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
title_full_unstemmed Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
title_sort Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121
dc.creator.none.fl_str_mv Baume, Gustavo Luis
Noël, N. E. D.
Costa, E.
Carraro, Giovanni
Méndez, R. A.
Pedreros, M. H.
author Baume, Gustavo Luis
author_facet Baume, Gustavo Luis
Noël, N. E. D.
Costa, E.
Carraro, Giovanni
Méndez, R. A.
Pedreros, M. H.
author_role author
author2 Noël, N. E. D.
Costa, E.
Carraro, Giovanni
Méndez, R. A.
Pedreros, M. H.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv Galaxies
Stars
Kron 11 (estrella)
Kron 63 (estrella)
NGC 121 (estrella)
topic Galaxies
Stars
Kron 11 (estrella)
Kron 63 (estrella)
NGC 121 (estrella)
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present observations for three star clusters, Kron 11, Kron 63 and NGC 121, in the Small Magellanic Cloud. We have studied their structure and derived their fundamental parameters by means of their luminosity functions, their colour magnitude diagrams and the Padova suite of isochrones. NGC 121 is a well-studied object, for which we confirm previous evidence about its old age and low-metal content, and have found that it is an undergoing mass segregation. Kron 11 and Kron 63 are poorly populated clusters which had never been studied so far. Kron 11 is several gigayears younger than NGC 121, while Kron 63 is basically a very young star aggregate. Both clusters are immersed in dense stellar fields which share the same population properties, suggesting that in their cases, cluster ages are consistent with typical ages of field stars.
Fil: Baume, Gustavo Luis. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentina
Fil: Noël, N. E. D.. Instituto de Astrofísica de Canarias; España
Fil: Costa, E.. Universidad de Chile; Chile
Fil: Carraro, Giovanni. European Southern Observatory; Chile
Fil: Méndez, R. A.. Universidad de Chile; Chile
Fil: Pedreros, M. H.. Universidad de Taracapà; Chile
description We present observations for three star clusters, Kron 11, Kron 63 and NGC 121, in the Small Magellanic Cloud. We have studied their structure and derived their fundamental parameters by means of their luminosity functions, their colour magnitude diagrams and the Padova suite of isochrones. NGC 121 is a well-studied object, for which we confirm previous evidence about its old age and low-metal content, and have found that it is an undergoing mass segregation. Kron 11 and Kron 63 are poorly populated clusters which had never been studied so far. Kron 11 is several gigayears younger than NGC 121, while Kron 63 is basically a very young star aggregate. Both clusters are immersed in dense stellar fields which share the same population properties, suggesting that in their cases, cluster ages are consistent with typical ages of field stars.
publishDate 2008
dc.date.none.fl_str_mv 2008-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/43218
Baume, Gustavo Luis; Noël, N. E. D.; Costa, E.; Carraro, Giovanni; Méndez, R. A.; et al.; Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 390; 12-2008; 1683-1690
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/43218
identifier_str_mv Baume, Gustavo Luis; Noël, N. E. D.; Costa, E.; Carraro, Giovanni; Méndez, R. A.; et al.; Basic parameters of three star clusters in the Small Magellanic Cloud: Kron 11, Kron 63 and NGC 121; Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 390; 12-2008; 1683-1690
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2008.13860.x
info:eu-repo/semantics/altIdentifier/url/https://onlinelibrary.wiley.com/toc/13652966/390/4
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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