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Large-Scale Variations in the Luminosity Function of Galaxies

  • Riccardo Giovanelli
  • Martha P. Haynes
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 141)

Abstract

We report observational evidence that the blue luminosity function depends on the local density of galaxies. While high luminosity galaxies are segregated to the high density regions, low luminosity ones are more diffusely distributed into regions of lower density contrast. This segregation, also seen in other properties such as surface brightness, supports the predictions of theories of biased galaxy formation and argues against the validity of a universal luminosity function (LF) for galaxies.

Keywords

Surface Brightness Luminosity Function Space Density High Density Region Velocity Interval 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • Riccardo Giovanelli
    • 1
    • 2
  • Martha P. Haynes
    • 1
    • 3
  1. 1.NAIC, Arecibo Observatory and Astronomy Dept.Cornell UniversityUSA
  2. 2.Arecibo ObservatoryUSA
  3. 3.Astronomy Dept., Space Sciences BuildingCornell UniversityIthacaUSA

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