Analysis of a complete sample of galaxies at m(Z) less than or equal to 14.5 - The optical, radio and far-infrared luminosity functions

Details Analysis of a complete sample of galaxies at m(Z) less than or equal to 14.5 - The optical, radio and far-infrared luminosity functions Analysis of a complete sample of galaxies at m(Z) less than or equal to 14.5 - The optical, radio and far-infrared luminosity functions

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.233..157f&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 233, July 1, 1988, p. 157-174. Research supported by th

Astronomy and Astrophysics

Astrophysics

40

Elliptical Galaxies, Galactic Radiation, Irregular Galaxies, Luminosity, Seyfert Galaxies, Spiral Galaxies, Starburst Galaxies, Astronomical Spectroscopy, Evolution (Development), Far Infrared Radiation, Galactic Radio Waves, Light Emission, Quasars, Spectral Bands

Scientific paper

As a first step towards a thorough analysis of evolution properties of galaxies in the optical, radio and far-IR bands, the authors have derived their local luminosity functions exploiting in particular a complete sample of 1671 galaxies observed in the Arecibo survey at 2.4 GHz and the IRAS data on them. The global luminosity functions have been analysed in terms of the contributions of four classes (normal spirals and irregulars; ellipticals and S0s; starburst/interacting; Seyferts) whose optical, far-IR and radio emissions are, at least partly, due to different astrophysical processes. Correlations between the luminosities in the three wavebands are discussed for each class.

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