Star formation histories of resolved stellar populations: in and beyond the Local Group

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dc.creatorTosi, Monica
dc.date2007-01-05
dc.date.accessioned2026-07-07T07:38:43Z
dc.date.available2026-07-07T07:38:43Z
dc.descriptionThe exploitation of the power and the spatial resolution of HST and new generation ground-based telescopes allows to measure with good precision the individual stars of galaxies in and beyond the Local Group. This leads to very successful studies of the star formation histories of galaxies of different morphological types. Our current knowledge of the star formation history of galaxies within 10-20 Mpc, as derived from the colour-magnitude diagrams of their resolved stellar populations, is reviewed here.
dc.description8 pages, 5 figs. Review presented at the meeting "From Stars to Galaxies" (Venezia, October 16-20 2006). To appear in ASP Conf.Ser., A.Vallenari, R.Tantalo, L.Portinari, A.Moretti eds
dc.identifierhttps://arxiv.org/abs/astro-ph/0701138
dc.identifierhttp://arxiv.org/abs/astro-ph/0701138
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121191
dc.subjectAstrophysics
dc.titleStar formation histories of resolved stellar populations: in and beyond the Local Group
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