Stellar evolution and variability in the pre-ZAHB phase

Monthly Notices of the Royal Astronomical Society

dc.creatorSilva-Aguirre, V.
dc.creatorCatelan, M.
dc.creatorValcarce, A.
dc.date2020-03-11T20:25:51Z
dc.date2022-07-07T23:42:54Z
dc.date2020-03-11T20:25:51Z
dc.date2022-07-07T23:42:54Z
dc.date2008
dc.date.accessioned2023-08-21T21:56:56Z
dc.date.available2023-08-21T21:56:56Z
dc.identifier15010003
dc.identifier15010003
dc.identifierhttps://hdl.handle.net/10533/237904
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8287419
dc.descriptionOne of the most dramatic events in the life of a low-mass star is the He flash, which takes place at the tip of the RGB and is followed by a series of secondary flashes before the star settles on the zero-age HB (ZAHB). Yet, no stars have ever been positi
dc.descriptionFONDAP
dc.descriptionFONDAP
dc.languageeng
dc.relationhttps://doi.org/10.1051/0004-6361:200810047
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.titleStellar evolution and variability in the pre-ZAHB phase
dc.titleMonthly Notices of the Royal Astronomical Society
dc.typeArticulo
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion


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