The Baade-Wesselink p-factor applicable to LMC Cepheids

Context. Recent observations of LMC Cepheids bring new constraints on the slope of the period-projection factor relation (hereafter Pp relation) that is currently used in the Baade-Wesselink (hereafter BW) method of distance determination. The discrepancy

Detalhes bibliográficos
Autores: Nardetto, N., Gieren, W., Pietrzynski, G.
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2011
País:Chile
Idioma:inglês
OAI Identifier:oai:repositorio.anid.cl:10533/240993
Acesso em linha:https://hdl.handle.net/10533/240993
Access Level:Acceso aberto
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spelling Pietrzynski, G.Gieren, W.Nardetto, N.201110.1051/0004-6361/201117459https://hdl.handle.net/10533/240993http://purl.org/coar/access_right/c_abf2The Baade-Wesselink p-factor applicable to LMC CepheidsNardetto, N.Gieren, W.Pietrzynski, G.2020-03-11T20:36:30Z2022-07-08T17:15:50Z2020-03-11T20:36:30Z2022-07-08T17:15:50Z2011Context. Recent observations of LMC Cepheids bring new constraints on the slope of the period-projection factor relation (hereafter Pp relation) that is currently used in the Baade-Wesselink (hereafter BW) method of distance determination. The discrepancyFONDAPFONDAP1501000315010003virtual::45707-1WOS:000296554800104https://hdl.handle.net/10533/240993eng10.1051/0004-6361/201117459https://doi.org/10.1051/0004-6361/201117459Atribución-NoComercial-SinDerivadas 3.0 Chilehttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/info:eu-repo/semantics/openAccessThe Baade-Wesselink p-factor applicable to LMC CepheidsAstronomy & AstrophysicsArticuloinfo:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttps://hdl.handle.net/10533/240993FONDAPhttp://purl.org/coar/resource_type/c_2df8fbb1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::45707-1045fc0e1-ef55-4532-8afe-69fe789d964dvirtual::45707-110533/240993oai:repositorio.anid.cl:10533/2409932023-07-24 18:03:36.78https://repositorio.anid.clRepositorio ANIDaletelier@anid.cl
dc.title.none.fl_str_mv The Baade-Wesselink p-factor applicable to LMC Cepheids
dc.title.journal.none.fl_str_mv Astronomy & Astrophysics
title The Baade-Wesselink p-factor applicable to LMC Cepheids
spellingShingle The Baade-Wesselink p-factor applicable to LMC Cepheids
Nardetto, N.
title_short The Baade-Wesselink p-factor applicable to LMC Cepheids
title_full The Baade-Wesselink p-factor applicable to LMC Cepheids
title_fullStr The Baade-Wesselink p-factor applicable to LMC Cepheids
title_full_unstemmed The Baade-Wesselink p-factor applicable to LMC Cepheids
title_sort The Baade-Wesselink p-factor applicable to LMC Cepheids
dc.creator.none.fl_str_mv Nardetto, N.
Gieren, W.
Pietrzynski, G.
author Nardetto, N.
author_facet Nardetto, N.
Gieren, W.
Pietrzynski, G.
author_role author
author2 Gieren, W.
Pietrzynski, G.
author2_role author
author
description Context. Recent observations of LMC Cepheids bring new constraints on the slope of the period-projection factor relation (hereafter Pp relation) that is currently used in the Baade-Wesselink (hereafter BW) method of distance determination. The discrepancy
publishDate 2011
dc.date.issued.none.fl_str_mv 2011
dc.date.accessioned.none.fl_str_mv 2020-03-11T20:36:30Z
2022-07-08T17:15:50Z
dc.date.available.none.fl_str_mv 2020-03-11T20:36:30Z
2022-07-08T17:15:50Z
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dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/10533/240993
identifier_str_mv 15010003
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url https://hdl.handle.net/10533/240993
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.doi.none.fl_str_mv 10.1051/0004-6361/201117459
dc.relation.uri.none.fl_str_mv https://doi.org/10.1051/0004-6361/201117459
dc.rights.none.fl_str_mv Atribución-NoComercial-SinDerivadas 3.0 Chile
http://creativecommons.org/licenses/by-nc-nd/3.0/cl/
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repository.name.fl_str_mv Repositorio ANID
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