The expected photometrical characteristics of high redshift spiral galaxies

Details The expected photometrical characteristics of high redshift spiral galaxies The expected photometrical characteristics of high redshift spiral galaxies

Apr 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010iaus..262..396m&link_type=abstract

Stellar Populations – Planning for the Next Decade, Proceedings of the International Astronomical Union, IAU Symposium, Volume 2

Astronomy and Astrophysics

Astronomy

Galaxies: Evolution, Galaxies: Photometry, Galaxies: Abundances

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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