Distance Scale, Variable Stars and Stellar Populations in Local Group Galaxies

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dc.creatorClementini, G.
dc.date2003-10-20
dc.date.accessioned2026-07-07T06:27:54Z
dc.date.available2026-07-07T06:27:54Z
dc.descriptionWe present an overview of our study of the short period variable stars in the Large Magellanic Cloud, and in the dwarf galaxies Fornax, Leo I, and NGC 6822. Light curves are presented for RR Lyrae stars, Anomalous Cepheids and, for the first time, for Dwarf Cepheids in the field and in the globular cluster #3 of the Fornax galaxy.
dc.description4 pages, 4 figures, Proceedings of the IAU Colloq. 193, "Variable Stars in the Local Group", ed. D. W. Kurtz & K. R. Pollard., ASP Conf. Ser., in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0310545
dc.identifierhttp://arxiv.org/abs/astro-ph/0310545
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/97553
dc.subjectAstrophysics
dc.titleDistance Scale, Variable Stars and Stellar Populations in Local Group Galaxies
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