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Optical, IR, and HI Observations of a Large Complete Cluster Sample

  • R. Brent Tully
  • Marc A. W. Verheijen
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 209)

Abstract

It is a chronic problem to achieve completeness in galaxy samples. Also, distance uncertainties confuse the comparison of properties between galaxies. These difficulties can be overcome by studying the members of clusters. The objects are essentially at the same distance and all objects that meet specified selection criteria within the volume of the cluster can be included. For example, a flux threshold might be set in some spectral band and this threshold corresponds to a specific absolute threshold for a complete sample.

Keywords

Star Formation Surface Brightness Luminosity Function Blue Edge Virgo Cluster 
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 1996

Authors and Affiliations

  • R. Brent Tully
    • 1
  • Marc A. W. Verheijen
    • 2
  1. 1.Institute for AstronomyUniversity of HawaiiHonoluluUSA
  2. 2.Kapteyn Astronomical InstituteGroningenThe Netherlands

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