Spectroscopic Dating of Stellar Populations from Local Star Clusters to Distant Galaxies and the Age of the Universe

dc.creatorA, Gustavo Bruzual
dc.date2002-02-08
dc.date.accessioned2026-07-25T11:42:53Z
dc.descriptionI summarize in terms of evolutionary population synthesis models our current understanding of stellar populations in different environments, from star clusters in nearby galaxies to distant galaxies in clusters or seen through gravitational lenses. Constraints on the age of the stellar populations in clusters and galaxies derived from comparing predicted and observed spectral energy distributions are examined and contrasted with the maximum ages allowed by cosmological models at the corresponding redshift.
dc.description5 pages, 5 figures, latex, macro included. To appear in the Proceedings of the 3rd Congress of the Venezuelan Physical Society in Revista Mexicana de Fisica, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0202178
dc.identifierhttp://arxiv.org/abs/astro-ph/0202178
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/5004
dc.subjectAstrophysics
dc.titleSpectroscopic Dating of Stellar Populations from Local Star Clusters to Distant Galaxies and the Age of the Universe
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