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“Downsizing” from the fossil record: Ages and metallicities of red galaxies and their dependence on mass and on environment
Published online by Cambridge University Press: 01 August 2006
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Red-sequence galaxies are known to obey well-defined scaling relations, such as the Fundamental Plane and the colour-magnitude relation, yet their star formation histories, which in part drive these relations, remain poorly understood. In this contribution, we summarize recent results from the NOAO Fundamental Plane Survey (NFPS). These results appear in more detail in Smith et al. (2006) and Nelan et al. (2005).
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 389 - 390
- Copyright
- Copyright © International Astronomical Union 2007
References
Nelan, J.E., Smith, R.J., Hudson, M.J., Wegner, G.A., Lucey, J.R., Moore, S.A.W., Quinney, S.J., & Suntzeff, N.B., 2005, ApJ, 632, 137CrossRefGoogle Scholar
Smith, R.J., Hudson, M.J., Lucey, J.R., Nelan, J.E., & Wegner, G.A., 2006, MNRAS, 369, 1419CrossRefGoogle Scholar
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