Fluorine Abundance Variations as a Signature of Enhanced Extra Mixing in Red Giants of the Globular Cluster M4

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dc.creatorDenissenkov, Pavel A.
dc.creatorPinsonneault, Marc
dc.creatorTerndrup, Donald M.
dc.date2006-04-24
dc.date.accessioned2026-07-07T10:43:54Z
dc.date.available2026-07-07T10:43:54Z
dc.descriptionWe show that enhanced extra mixing in low-mass red giants can result in a fluorine abundance that is correlated with abundance variations of other elements participating in H burning, such as C, N, O and Na. This finding is used to explain the fluorine abundance variations recently found in bright red giants of the globular cluster M4.
dc.description17 pages, 6 figures, submitted to ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0604503
dc.identifierhttp://arxiv.org/abs/astro-ph/0604503
dc.identifierAstrophys.J.651:438-443,2006
dc.identifierdoi:10.1086/507512
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182409
dc.subjectAstrophysics
dc.titleFluorine Abundance Variations as a Signature of Enhanced Extra Mixing in Red Giants of the Globular Cluster M4
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