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UV to NIR Galaxy Evolution and Galaxy Counts

Published online by Cambridge University Press:  25 May 2016

Michel Fioc
Michel Fioc*
Affiliation:
Institut d'Astrophysique de Paris, 98 bis, Bd. Arago, 75014 Paris, France

Extract

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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, cosmological ones might be put in evidence.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 373
Copyright
Copyright © Kluwer 1996