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The expected photometrical characteristics of high redshift spiral galaxies

Published online by Cambridge University Press:  13 April 2010

M. Mollá ,
M. García-Vargas  and
M. Martín-Manjón
M. Mollá
Affiliation:
Dpto. de Investigación Básica, CIEMAT, Avda. Complutense 22, 28040, Madrid (Spain) email: [email protected]
M. García-Vargas
Affiliation:
FRACTAL SLNE, C/ Tulipán 2, p13, 1A, 28231 Las Rozas de Madrid (Spain) email: [email protected]
M. Martín-Manjón
Affiliation:
Dpto. de Física Teórica, Universidad Autónoma de Madrid. 28049 Cantoblanco (Spain) email: [email protected]
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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.

Keywords

Galaxies: EvolutionGalaxies: PhotometryGalaxies: Abundances
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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