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UV to NIR Galaxy Evolution and Galaxy Counts

  • Michel Fioc
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 171)

Abstract

We have improved in the NIR the model of galaxy evolution developed by Guiderdoni & Rocca-Volmerange (A&A 186, 1) in the UV and the visible, allowing thus a multispectral analysis of the evolution of galaxies and of faint galaxy counts. Since evolutionnary effects should be low in the near-infrared, cosmologica! ones might be put in evidence.

Copyright information

© Springer Science+Business Media Dordrecht 1996

Authors and Affiliations

  • Michel Fioc
    • 1
  1. 1.Institut d’Astrophysique de ParisParisFrance

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