The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812

We have analyzed the double-lined eclipsing binary system OGLE-LMC-CEP-1812 in the LMC and demonstrate that it contains a classical fundamental mode Cepheid pulsating with a period of 1.31 days. The secondary star is a stable giant. We derive the dynamica

Detalhes bibliográficos
Autores: Pietrzynski, G., Gieren, W., Pilecki, B.
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2011
País:Chile
Idioma:inglés
OAI Identifier:oai:repositorio.anid.cl:10533/240994
Acesso em linha:https://hdl.handle.net/10533/240994
Access Level:acceso abierto
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spelling Pilecki, B.Gieren, W.Pietrzynski, G.201110.1088/2041-8205/742/2/L20https://hdl.handle.net/10533/240994http://purl.org/coar/access_right/c_abf2The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812Pietrzynski, G.Gieren, W.Pilecki, B.2020-03-11T20:36:30Z2022-07-08T17:15:51Z2020-03-11T20:36:30Z2022-07-08T17:15:51Z2011We have analyzed the double-lined eclipsing binary system OGLE-LMC-CEP-1812 in the LMC and demonstrate that it contains a classical fundamental mode Cepheid pulsating with a period of 1.31 days. The secondary star is a stable giant. We derive the dynamicaFONDAPFONDAP1501000315010003virtual::22503-1WOS:000296924700004https://hdl.handle.net/10533/240994eng10.1088/2041-8205/742/2/L20https://doi.org/10.1088/2041-8205/742/2/L20Atribución-NoComercial-SinDerivadas 3.0 Chilehttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/info:eu-repo/semantics/openAccessThe Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812Astrophysical Journal LettersArticuloinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttps://hdl.handle.net/10533/240994FONDAPhttp://purl.org/coar/resource_type/c_2df8fbb1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::22503-1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::22503-110533/240994oai:repositorio.anid.cl:10533/2409942023-07-24 20:27:02.524https://repositorio.anid.clRepositorio ANIDaletelier@anid.cl
dc.title.none.fl_str_mv The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
dc.title.journal.none.fl_str_mv Astrophysical Journal Letters
title The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
spellingShingle The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
Pietrzynski, G.
title_short The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
title_full The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
title_fullStr The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
title_full_unstemmed The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
title_sort The Araucaria Project: Accurate Determination of the Dynamical Mass of the Classical Cepheid in the Eclipsing System OGLE-LMC-CEP-1812
dc.creator.none.fl_str_mv Pietrzynski, G.
Gieren, W.
Pilecki, B.
author Pietrzynski, G.
author_facet Pietrzynski, G.
Gieren, W.
Pilecki, B.
author_role author
author2 Gieren, W.
Pilecki, B.
author2_role author
author
description We have analyzed the double-lined eclipsing binary system OGLE-LMC-CEP-1812 in the LMC and demonstrate that it contains a classical fundamental mode Cepheid pulsating with a period of 1.31 days. The secondary star is a stable giant. We derive the dynamica
publishDate 2011
dc.date.issued.none.fl_str_mv 2011
dc.date.accessioned.none.fl_str_mv 2020-03-11T20:36:30Z
2022-07-08T17:15:51Z
dc.date.available.none.fl_str_mv 2020-03-11T20:36:30Z
2022-07-08T17:15:51Z
dc.type.none.fl_str_mv Articulo
dc.type.driver.none.fl_str_mv info:eu-repo/semantics/article
dc.type.openaire.none.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.folio.none.fl_str_mv 15010003
15010003
dc.identifier.idwos.none.fl_str_mv WOS:000296924700004
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10533/240994
identifier_str_mv 15010003
WOS:000296924700004
url https://hdl.handle.net/10533/240994
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.doi.none.fl_str_mv 10.1088/2041-8205/742/2/L20
dc.relation.uri.none.fl_str_mv https://doi.org/10.1088/2041-8205/742/2/L20
dc.rights.none.fl_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rights.driver.none.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
eu_rights_str_mv openAccess
repository.name.fl_str_mv Repositorio ANID
repository.mail.fl_str_mv aletelier@anid.cl
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