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J.H. Howell (UC Santa Cruz)
High signal-to-noise spectroscopic observations are presented of both a volume-limited sample of nearby elliptical galaxies as well as a separate sample of suspected merger remnant ellipticals. The results of a detailed stellar population analysis are presented, examining the correlations between age, metallicity, [\alpha Fe], and other galaxy properties.
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Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.