Two extreme contact binary systems in the nearest globular cluster M4

Autores
Liu, L.; Qian, S. B.; Fernandez Lajus, Eduardo Eusebio
Año de publicación
2011
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q =0.123 ±0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q =1.230 ±0.004), deep-contact (f =79.7 ±1.9 per cent) system. It is also a blue straggler.
Fil: Liu, L.. Chinese Academy Of Sciences; República de China
Fil: Qian, S. B.. Chinese Academy Of Sciences; República de China
Fil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina; Argentina
Materia
Eclipsing Binaries
V53 (Estrella)
V47 (Estrella)
Evolution of Stars
Blue Stragglers
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:11336/16410
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/16410
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Two extreme contact binary systems in the nearest globular cluster M4Liu, L.Qian, S. B.Fernandez Lajus, Eduardo EusebioEclipsing BinariesV53 (Estrella)V47 (Estrella)Evolution of StarsBlue Stragglershttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q =0.123 ±0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q =1.230 ±0.004), deep-contact (f =79.7 ±1.9 per cent) system. It is also a blue straggler.Fil: Liu, L.. Chinese Academy Of Sciences; República de ChinaFil: Qian, S. B.. Chinese Academy Of Sciences; República de ChinaFil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina; ArgentinaOxford University Press2011-07info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16410Liu, L.; Qian, S. B.; Fernandez Lajus, Eduardo Eusebio; Two extreme contact binary systems in the nearest globular cluster M4; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 415; 2; 7-2011; 1509-15220035-87111365-2966enginfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2011.18791.xinfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.18791.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:34:04Zoai:ri.conicet.gov.ar:11336/16410instacron: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 09:34:04.663CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Two extreme contact binary systems in the nearest globular cluster M4
title Two extreme contact binary systems in the nearest globular cluster M4
spellingShingle Two extreme contact binary systems in the nearest globular cluster M4
Liu, L.
Eclipsing Binaries
V53 (Estrella)
V47 (Estrella)
Evolution of Stars
Blue Stragglers
title_short Two extreme contact binary systems in the nearest globular cluster M4
title_full Two extreme contact binary systems in the nearest globular cluster M4
title_fullStr Two extreme contact binary systems in the nearest globular cluster M4
title_full_unstemmed Two extreme contact binary systems in the nearest globular cluster M4
title_sort Two extreme contact binary systems in the nearest globular cluster M4
dc.creator.none.fl_str_mv Liu, L.
Qian, S. B.
Fernandez Lajus, Eduardo Eusebio
author Liu, L.
author_facet Liu, L.
Qian, S. B.
Fernandez Lajus, Eduardo Eusebio
author_role author
author2 Qian, S. B.
Fernandez Lajus, Eduardo Eusebio
author2_role author
author
dc.subject.none.fl_str_mv Eclipsing Binaries
V53 (Estrella)
V47 (Estrella)
Evolution of Stars
Blue Stragglers
topic Eclipsing Binaries
V53 (Estrella)
V47 (Estrella)
Evolution of Stars
Blue Stragglers
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 the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q =0.123 ±0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q =1.230 ±0.004), deep-contact (f =79.7 ±1.9 per cent) system. It is also a blue straggler.
Fil: Liu, L.. Chinese Academy Of Sciences; República de China
Fil: Qian, S. B.. Chinese Academy Of Sciences; República de China
Fil: Fernandez Lajus, Eduardo Eusebio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto de Astrofísica de la Plata; Argentina; Argentina
description We present the results of photometric solutions for two contact binaries in the nearby globular cluster M4. We estimate their physical parameters using the light-curve program of the Wilson Devinney code. These systems have quite different mass ratios, which indicates that they did not form at the same time. V47 is an extreme mass-ratio system (q =0.123 ±0.002) being dissimilar to the same kind of field contact binaries. V53 is a high mass-ratio (q =1.230 ±0.004), deep-contact (f =79.7 ±1.9 per cent) system. It is also a blue straggler.
publishDate 2011
dc.date.none.fl_str_mv 2011-07
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/11336/16410
Liu, L.; Qian, S. B.; Fernandez Lajus, Eduardo Eusebio; Two extreme contact binary systems in the nearest globular cluster M4; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 415; 2; 7-2011; 1509-1522
0035-8711
1365-2966
url http://hdl.handle.net/11336/16410
identifier_str_mv Liu, L.; Qian, S. B.; Fernandez Lajus, Eduardo Eusebio; Two extreme contact binary systems in the nearest globular cluster M4; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 415; 2; 7-2011; 1509-1522
0035-8711
1365-2966
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1365-2966.2011.18791.x
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-lookup/doi/10.1111/j.1365-2966.2011.18791.x
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 Oxford University Press
publisher.none.fl_str_mv Oxford University Press
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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score 13.070432

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