The expected photometrical characteristics of high redshift spiral galaxies

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics

Scientific paper

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2 pages, 1 figure, to be published in the proceedings of IAU Symp. 262 "Stellar Populations - Planing for the Next Decate" (Au

Scientific paper

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.

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