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Three-color CCD photometry of the distant cluster of galaxies Cl 0024 + 1654Photometry of 265 galaxies in rich cluster Cl 0024 + 1654 (z = 0.39), based on CCD imaging in three filters, is presented. The luminosity of this system ranks it among the richest known clusters, and it has a blue mass-to-light ratio of about 210. The color-magnitude diagram has a prominent E/S0 sequence. There are essentially no blue cluster members brighter than r equals about 19.3, and only very red galaxies inhabit the central 30 arcsec of the cluster. The blue cluster members have sizes and surface brightnesses similar to spiral galaxies in nearby clusters.
Document ID
19870027177
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schneider, D. P.
(Palomar Observatory, Pasadena, CA; Institute for Advanced Study, Princeton NJ, United States)
Dressler, A.
(Mount Wilson and Las Campanas Observatories Pasadena, CA, United States)
Gunn, J. E.
(Princeton University Observatory, NJ, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1986
Publication Information
Publication: Astronomical Journal
Volume: 92
ISSN: 0004-6256
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-6256
Accession Number
87A14451
Funding Number(s)
CONTRACT_GRANT: NAS5-29225
CONTRACT_GRANT: NSF AST-83-14134
Distribution Limits
Public
Copyright
Other

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