Ages and chemical properties of stellar populations from integrated spectra and spectral indexes

Details Ages and chemical properties of stellar populations from integrated spectra and spectral indexes Ages and chemical properties of stellar populations from integrated spectra and spectral indexes

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111...39v&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

Physics

1

Protogalaxies, Primordial Galaxies, Accretion And Accretion Disks, Star Formation

Scientific paper

The various methods for studying in detail relevant stellar population parameters throught the integrated light are reviewed. The emphasis is given to the analysis based on absorption line-strength indices. The state-of-the-art of the stellar population synthesis models and methodologies is summarized. Finally some of the various uncertainties and limitations, which are lurking these studies are shown and discussed.

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