Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation

Autores
Gonzalez, Jorge Federico; Ostrov, Pablo Gabriel; Morrell, Nidia Irene; Minniti, Dante
Año de publicación
2005
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
A simultaneous light and radial velocity analysis of eight Large Magellanic Cloud (LMC) eclipsing binaries is presented. Combining spectroscopic observations obtained with UVES at the ESO Very Large Telescope and light curves available from the MACHO and OGLE databases, accurate masses and radii for the binary components, along with their spectral types and luminosities, are derived. These determinations allow us to construct the first mass-luminosity relation for late O and early B type stars in the LMC. This mass-luminosity relation looks very similar to that of the Milky Way, in spite of the different metallicities. The good agreement achieved in the comparison with recent theoretical isochrones is encouraging regarding the reliability of star models up to 20 M⊙.
Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Ostrov, Pablo Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Morrell, Nidia Irene. Universidad Nacional de La Plata; Argentina. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Minniti, Dante. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile
Materia
BINARIES: ECLIPSING
MAGELLANIC CLOUDS
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
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:11336/213799
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relationGonzalez, Jorge FedericoOstrov, Pablo GabrielMorrell, Nidia IreneMinniti, DanteBINARIES: ECLIPSINGMAGELLANIC CLOUDSSTARS: EARLY-TYPESTARS: FUNDAMENTAL PARAMETERShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1A simultaneous light and radial velocity analysis of eight Large Magellanic Cloud (LMC) eclipsing binaries is presented. Combining spectroscopic observations obtained with UVES at the ESO Very Large Telescope and light curves available from the MACHO and OGLE databases, accurate masses and radii for the binary components, along with their spectral types and luminosities, are derived. These determinations allow us to construct the first mass-luminosity relation for late O and early B type stars in the LMC. This mass-luminosity relation looks very similar to that of the Milky Way, in spite of the different metallicities. The good agreement achieved in the comparison with recent theoretical isochrones is encouraging regarding the reliability of star models up to 20 M⊙.Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Ostrov, Pablo Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; ArgentinaFil: Morrell, Nidia Irene. Universidad Nacional de La Plata; Argentina. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; ArgentinaFil: Minniti, Dante. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; ChileIOP Publishing2005-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/213799Gonzalez, Jorge Federico; Ostrov, Pablo Gabriel; Morrell, Nidia Irene; Minniti, Dante; Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation; IOP Publishing; Astrophysical Journal; 624; 2 I; 12-2005; 946-9560004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1086/428920info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/428920info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:43:52Zoai:ri.conicet.gov.ar:11336/213799instacron: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:34982025-09-03 09:43:53.056CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
title Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
spellingShingle Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
Gonzalez, Jorge Federico
BINARIES: ECLIPSING
MAGELLANIC CLOUDS
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
title_short Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
title_full Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
title_fullStr Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
title_full_unstemmed Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
title_sort Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation
dc.creator.none.fl_str_mv Gonzalez, Jorge Federico
Ostrov, Pablo Gabriel
Morrell, Nidia Irene
Minniti, Dante
author Gonzalez, Jorge Federico
author_facet Gonzalez, Jorge Federico
Ostrov, Pablo Gabriel
Morrell, Nidia Irene
Minniti, Dante
author_role author
author2 Ostrov, Pablo Gabriel
Morrell, Nidia Irene
Minniti, Dante
author2_role author
author
author
dc.subject.none.fl_str_mv BINARIES: ECLIPSING
MAGELLANIC CLOUDS
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
topic BINARIES: ECLIPSING
MAGELLANIC CLOUDS
STARS: EARLY-TYPE
STARS: FUNDAMENTAL PARAMETERS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv A simultaneous light and radial velocity analysis of eight Large Magellanic Cloud (LMC) eclipsing binaries is presented. Combining spectroscopic observations obtained with UVES at the ESO Very Large Telescope and light curves available from the MACHO and OGLE databases, accurate masses and radii for the binary components, along with their spectral types and luminosities, are derived. These determinations allow us to construct the first mass-luminosity relation for late O and early B type stars in the LMC. This mass-luminosity relation looks very similar to that of the Milky Way, in spite of the different metallicities. The good agreement achieved in the comparison with recent theoretical isochrones is encouraging regarding the reliability of star models up to 20 M⊙.
Fil: Gonzalez, Jorge Federico. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Ostrov, Pablo Gabriel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - San Juan. Complejo Astronómico "El Leoncito". Universidad Nacional de Córdoba. Complejo Astronómico "El Leoncito". Universidad Nacional de la Plata. Complejo Astronómico "El Leoncito". Universidad Nacional de San Juan. Complejo Astronómico "El Leoncito"; Argentina
Fil: Morrell, Nidia Irene. Universidad Nacional de La Plata; Argentina. Las Campanas Observatory; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata; Argentina
Fil: Minniti, Dante. Pontificia Universidad Católica de Chile; Chile. Universidad Católica de Chile; Chile
description A simultaneous light and radial velocity analysis of eight Large Magellanic Cloud (LMC) eclipsing binaries is presented. Combining spectroscopic observations obtained with UVES at the ESO Very Large Telescope and light curves available from the MACHO and OGLE databases, accurate masses and radii for the binary components, along with their spectral types and luminosities, are derived. These determinations allow us to construct the first mass-luminosity relation for late O and early B type stars in the LMC. This mass-luminosity relation looks very similar to that of the Milky Way, in spite of the different metallicities. The good agreement achieved in the comparison with recent theoretical isochrones is encouraging regarding the reliability of star models up to 20 M⊙.
publishDate 2005
dc.date.none.fl_str_mv 2005-12
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/11336/213799
Gonzalez, Jorge Federico; Ostrov, Pablo Gabriel; Morrell, Nidia Irene; Minniti, Dante; Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation; IOP Publishing; Astrophysical Journal; 624; 2 I; 12-2005; 946-956
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/213799
identifier_str_mv Gonzalez, Jorge Federico; Ostrov, Pablo Gabriel; Morrell, Nidia Irene; Minniti, Dante; Absolute parameters for eight eclipsing binaries in the large magellanic cloud: The mass-luminosity relation; IOP Publishing; Astrophysical Journal; 624; 2 I; 12-2005; 946-956
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1086/428920
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1086/428920
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
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
_version_ 1842268629575401472
score 13.13397

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