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The expected photometrical characteristics of high redshift spiral galaxies

Published online by Cambridge University Press:  13 April 2010

M. Mollá
Affiliation:
Dpto. de Investigación Básica, CIEMAT, Avda. Complutense 22, 28040, Madrid (Spain) email: mercedes.molla@ciemat.es
M. García-Vargas
Affiliation:
FRACTAL SLNE, C/ Tulipán 2, p13, 1A, 28231 Las Rozas de Madrid (Spain) email: marisa.garcia@fractal-es.com
M. Martín-Manjón
Affiliation:
Dpto. de Física Teórica, Universidad Autónoma de Madrid. 28049 Cantoblanco (Spain) email: mariluz.martin@uam.es
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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.

Type
Poster Papers
Copyright
Copyright © International Astronomical Union 2010

References

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