Modelling evolution of stellar emission of galaxies for the NIR surveys

Details Modelling evolution of stellar emission of galaxies for the NIR surveys Modelling evolution of stellar emission of galaxies for the NIR surveys

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.217..273r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 217, no. 1-2, p. 273-278

Astronomy and Astrophysics

Astronomy

Chronology, Galactic Evolution, Near Infrared Radiation, Radio Galaxies, Sky Surveys (Astronomy), Starburst Galaxies, Ultraviolet Emission, Infrared Astronomy, Light (Visible Radiation), Populations, Red Shift, Spectral Energy Distribution, Stellar Spectrophotometry, Ultraviolet Radiation

Scientific paper

Recent observational results in the near-IR on distant galaxies and interacting galaxies are clues for modelling evolution of galaxy counts and for testing theories of galaxy formation. Spectrophotometric models, developed in the ultraviolet and visible, were tools essential for such interpretations. So, we hereafter present their extension to the near-infrared and preliminary results on radiogalaxies, starbursts and faint counts. The two fundamental objectives are to confirm a merging scenario and to determine the age of the first stellar generation.

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