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The General Galaxy Luminosity Function
Published online by Cambridge University Press: 03 August 2017
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The general luminosity function of galaxies is believed to be well represented by the Schechter function with exponent α ≃ −1 and L* ≃ 1010L⊙, but with a wide range of variation from one sample to another. This function decreases exponentially at high luminosities and has a power law behaviour increasing towards low luminosities with no present evidence of turn over or cut-off.
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- Appendix 1: Poster Papers
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- Copyright © Reidel 1988
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