Abstract
Integrated broad-band colors and metallic lines cannot discriminate clearly between the effects of age and Z in old stellar populations. Such data are more sensitive to Z than to age. The Hβ feature provides a way to break this degeneracy. New measurements indicate that the mean stellar ages of typical E galaxy nuclei are fairly young, ranging from 2 to ∼12 Gyr. The outer parts of E galaxies are both older and more metal-poor than nuclei, consistent with the formation of E galaxies via mergers and starbursts. Age effects contribute strongly to the classic color-line strength sequence of E galaxies.
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Faber, S.M., Trager, S.C., Gonzalez, J.J., Worthey, G. (1995). The Stellar Ages of Elliptical Galaxies. In: van der Kruit, P.C., Gilmore, G. (eds) Stellar Populations. International Astronomical Union / Union Astronomique Internationale, vol 164. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0125-7_23
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DOI: https://doi.org/10.1007/978-94-011-0125-7_23
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