­

IPAC

Home

NASA/IPAC Extragalactic Database

  • Home
  • Search Objects »
    • By Name
    • Near Name or Position (Cone)
    • In Refcode
    • By Parameters
  • Literature »
    • References by Author Name
    • Reference Lookup
    • Nomenclature
  • Services »
    • Gravitational Wave Followup » »
      • Overview
      • Events
    • Ticket Status
    • Level5 » »
      • Knowledge Base
      • Glossary
    • Classic Home Page
  • Tools »
    • Coordinate Calculator
    • Extinction Calculator
    • Velocity Calculator
  • Information »
    • Overview » »
      • News
      • Archived Release Notes
    • User Guides » »
      • Search Objects
      • Calculators
      • Program Interfaces
      • Database
      • Tutorials
      • Best Practices
      • Search & Retrieval FAQ
      • Scientific Calculations FAQ
      • Known Issues
      • Discontinuing Services
    • Holdings » »
      • Nomenclature
      • Counts
      • Graphics
      • Data Sets
    • References » »
      • Articles about NED
      • Brochure (pdf)
      • Cosmology Calculators
      • Extinction-Law Calculators
      • Related Sites
    • Community » »
      • Users Committee
      • Ambassadors
    • Team
    • Contact Us

You are here

Home » Literature » Reference Lookup

Help Reference Information

TitleThe Velocity Dispersion Function of Very Massive Galaxy Clusters: Abell 2029 and Coma
AuthorsSohn, Jubee; Geller, Margaret J.; Zahid, H. Jabran; Fabricant, Daniel G.; Diaferio, Antonaldo; Rines, Kenneth J.
Bibcode

2017ApJS..229...20S   Search ADS ↗

AbstractBased on an extensive redshift survey for galaxy clusters Abell 2029 and Coma, we measure the luminosity functions (LFs) and stellar mass functions (SMFs) for the entire cluster member galaxies. Most importantly, we measure the velocity dispersion functions (VDFs) for quiescent members. The MMT/Hectospec redshift survey for galaxies in A2029 identifies 982 spectroscopic members; for 838 members, we derive the central velocity dispersion from the spectroscopy. Coma is the only other cluster surveyed as densely. The LFs, SMFs, and VDFs for A2029 and Coma are essentially identical. The SMFs of the clusters are consistent with simulations. The A2029 and Coma VDFs for quiescent galaxies have a significantly steeper slope than those of field galaxies for velocity dispersion ≲ 100 {km} {{{s}}}-1. The cluster VDFs also exceed the field at velocity dispersion ≳ 250 {km} {{{s}}}-1. The differences between cluster and field VDFs are potentially important tests of simulations and of the formation of structure in the universe.
Objects

984 Objects    Search NED ↙

Reload form

The NASA/IPAC Extragalactic Database (NED) is funded by the
National Aeronautics and Space Administration under
Award Number 80NSSC21M0037, and operated by the California Institute of Technology.

  • IPAC
  • Caltech
  • NASA
  • About NED
  • Acknowledging NED
  • Connect with NED:
    • EMail
    • facebook
    • youtube
Copyright © 2025, California Institute of Technology
back up ↑