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Stellar Population SEDs at 2.3Å
Published online by Cambridge University Press: 01 December 2006
Abstract
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We present a new spectral library for old and intermediate-aged single-age, single-metallicity stellar populations for a wide metallicity range. The major ingredient of these models is a new empirical stellar library composed of 985 stars, whose main characteristic is its unprecedented stellar atmospheric parameters coverage. The model SEDs cover the spectral range 3540-7410A at 2.3A (FWHM). We present some advantages and applications of these models.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S241: Stellar Populations as Building Blocks of Galaxies , December 2006 , pp. 133 - 137
- Copyright
- Copyright © International Astronomical Union 2007
References
Cenarro, J., Gorgas, J., Cardiel, N., Vazdekis, A., & Peletier, R. 2002, MNRAS 329, 863CrossRefGoogle Scholar
Vazdekis, A., Cenarro, J., Gorgas, J., Cardiel, N., & Peletier, R. 2003, MNRAS 340, 1317CrossRefGoogle Scholar
Vazdekis, A., Kuntschner, H., Davies, R.L., Arimoto, N., Nakamura, O., Peletier, R. 2001, ApJ 551, L127CrossRefGoogle Scholar
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