Absolute parameters for eight eclipsing binaries in the Large Magellanic Cloud: The mass-luminosity relation

Autores
González, 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⊙.
Facultad de Ciencias Astronómicas y Geofísicas
Materia
Ciencias Astronómicas
Binaries: Eclipsing
Magellanic clouds
Stars: Early-type
Stars: Fundamental parameters
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:10915/83385
Acceder
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oai_identifier_str oai:sedici.unlp.edu.ar:10915/83385
network_acronym_str SEDICI
repository_id_str 1329
network_name_str SEDICI (UNLP)
spelling Absolute parameters for eight eclipsing binaries in the Large Magellanic Cloud: The mass-luminosity relationGonzález, Jorge FedericoOstrov, Pablo GabrielMorrell, Nidia IreneMinniti, DanteCiencias AstronómicasBinaries: EclipsingMagellanic cloudsStars: Early-typeStars: Fundamental parametersA 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⊙.Facultad de Ciencias Astronómicas y Geofísicas2005info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdf946-956http://sedici.unlp.edu.ar/handle/10915/83385enginfo:eu-repo/semantics/altIdentifier/issn/0004-637Xinfo:eu-repo/semantics/altIdentifier/doi/10.1086/428920info: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:UNLP2025-10-22T16:56:37Zoai:sedici.unlp.edu.ar:10915/83385Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 16:56:38.211SEDICI (UNLP) - Universidad Nacional de La Platafalse
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
González, Jorge Federico
Ciencias Astronómicas
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 González, Jorge Federico
Ostrov, Pablo Gabriel
Morrell, Nidia Irene
Minniti, Dante
author González, Jorge Federico
author_facet González, 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 Ciencias Astronómicas
Binaries: Eclipsing
Magellanic clouds
Stars: Early-type
Stars: Fundamental parameters
topic Ciencias Astronómicas
Binaries: Eclipsing
Magellanic clouds
Stars: Early-type
Stars: Fundamental parameters
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⊙.
Facultad de Ciencias Astronómicas y Geofísicas
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
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/83385
url http://sedici.unlp.edu.ar/handle/10915/83385
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0004-637X
info:eu-repo/semantics/altIdentifier/doi/10.1086/428920
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)
dc.format.none.fl_str_mv application/pdf
946-956
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
instacron:UNLP
reponame_str SEDICI (UNLP)
collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
instacron_str UNLP
institution UNLP
repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
repository.mail.fl_str_mv alira@sedici.unlp.edu.ar
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score 12.982451

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