K-corrections for galaxies of different morphological types

Details K-corrections for galaxies of different morphological types K-corrections for galaxies of different morphological types

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203...39p&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 1, 1976, pt. 1, p. 39-51.

Astronomy and Astrophysics

Astrophysics

324

Astronomical Photometry, Red Shift, Spectral Energy Distribution, Ubv Spectra, Astronomical Catalogs, Colorimetry, Frequency Ranges, Galactic Evolution, Oao 2, Tables (Data)

Scientific paper

Mean energy distributions from 1500 to 8000 A for different types of galaxies have been derived from satellite ultraviolet-filter photometry and from earth-based spectrum scans. K-corrections for the standard U, B, V filters have been calculated from these energy distributions. The K-corrections are used to calculate the mean redshift, mean observed color, and color distribution of galaxies as a function of apparent magnitude and type in a Euclidean universe, assuming no galaxy evolution and no intergalactic extinction.

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