Calibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC

Astronomy & Astrophysics

dc.creatorStorm, J.
dc.creatorGieren, W.
dc.creatorPietrzyński, G.
dc.creatorFouqué, P.
dc.creatorBarnes, T. G.
dc.creatorSoszyński, I.
dc.creatorNardetto, N.
dc.creatorQueloz, D.
dc.date2020-03-11T20:36:47Z
dc.date2022-07-08T17:17:35Z
dc.date2020-03-11T20:36:47Z
dc.date2022-07-08T17:17:35Z
dc.date2011
dc.date.accessioned2023-08-23T00:37:01Z
dc.date.available2023-08-23T00:37:01Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/241092
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8355808
dc.descriptionThe extragalactic distance scale builds directly on the Cepheid Period-Luminosity (PL) relation as delineated by the sample of Cepheids in the Large Magellanic Cloud (LMC). However, the LMC is a dwarf irregular galaxy, quite different from the massive spi
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361/201117154
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.titleCalibrating the Cepheid period-luminosity relation from the infrared surface brightness technique. II. The effect of metallicity and the distance to the LMC
dc.titleAstronomy & Astrophysics
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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