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The expected photometrical characteristics of high redshift spiral galaxies
Published online by Cambridge University Press: 13 April 2010
Abstract
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The star formation and the subsequent metallic enrichment of spiral galaxies, occurring at the early phases of their evolution, produce emission lines whose contribution may change the colors of these objects. We have computed this contribution with consistent chemo-spectro-photometrical theoretical models in order to calculate the variations in the colors evolution.
- Type
- Poster Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 396 - 397
- Copyright
- Copyright © International Astronomical Union 2010
References
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Martín-Manjón, M. L., García-Vargas, M. L., Mollá, M., & Díaz, A. I. 2009, MNRAS, submitted (Paper II)Google Scholar
Mollá, M., García-Vargas, M. L., & Bressan, A. 2009, MNRAS, 398, 451 (Paper I)CrossRefGoogle Scholar
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