Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...300..151l&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 300, Jan. 1, 1986, p. 151-158. NSF-supported research.
Astronomy and Astrophysics
Astrophysics
31
Astronomical Photometry, Elliptical Galaxies, Galactic Evolution, Infrared Photometry, Luminosity, Luminous Intensity, Near Infrared Radiation, Radio Galaxies, Red Shift, Visible Spectrum
Scientific paper
Near-infrared photometry for 61 elliptical galaxies is used with previously published data to demonstrate that little or no color evolution is observed at infrared wavelengths, while galaxies near z = 1 are brighter than those at low redshift. Optically selected galaxies are compared with radio galaxies, and no differences in infrared properties are found. Evolution of a stellar population with an initial mass function similar to that observed in the solar neighborhood coupled with a value for q0 near 0.5 provides the best fit to the color and luminosity data.
Eisenhardt Peter R. M.
Lebofsky Marcia J.
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