Stellar Content and Star Formation Histories

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dc.creatorTosi, M.
dc.date1993-12-14
dc.date.accessioned2026-07-07T02:19:01Z
dc.date.available2026-07-07T02:19:01Z
dc.descriptionThe evolution of irregular galaxies is examined from two points of view: on the one hand, models of galactic chemical evolution have been computed and their predictions compared with the corresponding observational data on the element abundances, and on the other hand, the results of a new method to derive the star formation history in the last 1 Gyr in nearby irregulars are presented.
dc.descriptionplaine TEX, the postscript files for the figures are appended at the end of the TEX file, BAP12-1993-041-OAB
dc.identifierhttps://arxiv.org/abs/astro-ph/9312030
dc.identifierhttp://arxiv.org/abs/astro-ph/9312030
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9708
dc.subjectAstrophysics
dc.titleStellar Content and Star Formation Histories
dc.typetext

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