Bivariate luminosity function of E and S0 galaxies

Details Bivariate luminosity function of E and S0 galaxies Bivariate luminosity function of E and S0 galaxies

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214..197c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 15, 1985, p. 197-202.

Statistics

Computation

23

Bivariate Analysis, Brightness Distribution, Elliptical Galaxies, Functions (Mathematics), Luminosity, Spiral Galaxies, Computational Astrophysics, Galactic Structure, Radii

Scientific paper

A function which describes the joint distribution of luminosity and
radius of galaxies - the bivariate luminosity function (BLF) is defined.
A simple analytical formula for the shape of BLF is proposed and fitted
to the data for E and S0 galaxies from the sample of Sadler (1984).

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