Abstract
The stellar population properties of elliptical galaxies are examined using a homogeneous, distance-independent set of parameters for over 400 ellipticals. The relationship between (B-V) color and the Mg2 index shows little evidence of cosmic scatter, despite the fact that the color is measured in a signficantly larger aperture. However, the relationship between Mg2 and central velocity dispersion, σ, does show evidence for a significant subset of ellipticals having weaker values of Mg2 for their values of σ.
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References
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© 1988 Kluwer Academic Publishers
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Burstein, D. et al. (1988). Global Stellar Populations of Elliptical Galaxies: A. Optical Properties. In: Kron, R.G., Renzini, A. (eds) Towards Understanding Galaxies at Large Redshift. Astrophysics and Space Science Library, vol 141. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2919-7_3
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DOI: https://doi.org/10.1007/978-94-009-2919-7_3
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7814-6
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