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
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/83385
Ver los metadatos del registro completo
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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:UNLP2025-09-29T11:15:46Zoai: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:13292025-09-29 11:15:46.974SEDICI (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 |
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reponame:SEDICI (UNLP) instname:Universidad Nacional de La Plata instacron:UNLP |
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Universidad Nacional de La Plata |
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SEDICI (UNLP) - Universidad Nacional de La Plata |
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alira@sedici.unlp.edu.ar |
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