Stellar Populations and Chemical Evolution of Late--Type Dwarf Galaxies

Simple item page
dc.creatorTosi, M.
dc.date2001-04-02
dc.date.accessioned2026-07-07T01:58:06Z
dc.date.available2026-07-07T01:58:06Z
dc.descriptionSome aspects of the chemical evolution of late-type dwarf galaxies are reviewed, together with their implications on three issues of cosmological relevance: similarity to primeval galaxies, derivation of the primordial helium abundance, contribution to the excess of faint blue galaxies. A more detailed approach to model their evolution is suggested. The importance of deriving the star formation history in these systems by studying their resolved stellar populations is emphasized.
dc.description8 pages, 6 encapsulated figs. Review paper to appear in 'Dwarf Galaxies and their Environment", K.S. de Boer, R.J. Dettmar, U. Klein eds (Shaker Verlag, De), 2001 in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0104016
dc.identifierhttp://arxiv.org/abs/astro-ph/0104016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2641
dc.subjectAstrophysics
dc.titleStellar Populations and Chemical Evolution of Late--Type Dwarf Galaxies
dc.typetext

Files

Collections

arXiv