Age-metallicity relation and Chemical evolution of the LMC from UVES spectra of Globular Cluster giants

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dc.creatorHill, V.
dc.creatorFrançois, P.
dc.creatorSpite, M.
dc.creatorPrimas, F.
dc.creatorSpite, F.
dc.date2000-09-18
dc.date.accessioned2026-07-07T01:55:29Z
dc.date.available2026-07-07T01:55:29Z
dc.descriptionWe report on the first high-resolution spectroscopy of 10 giants in LMC Globular Clusters in a wide age range, obtained with the newly commissioned spectrograph UVES at VLT UT2. These observations are used to derive oxygen and iron content of these clusters, and the abundances are then used to cast a more precise view, not only on the age-metallicity relation in the LMC, but also on the chemical evolution of this dwarf irregular galaxy.
dc.descriptionAccepted in Astronomy&Astrophysics, 7 pages, 9 Postscript figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0009273
dc.identifierhttp://arxiv.org/abs/astro-ph/0009273
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1671
dc.subjectAstrophysics
dc.titleAge-metallicity relation and Chemical evolution of the LMC from UVES spectra of Globular Cluster giants
dc.typetext

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