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The Galaxy Populations of Clusters at High Redshifts: A “Hubble Atlas”

Published online by Cambridge University Press:  25 May 2016

S.C. Trager ,
S.M. Faber ,
A. Dressler  and
The WF/PC-I Instrument Definition Team
S.C. Trager
Affiliation:
UCO/Lick Observatory, Santa Cruz, CA 95064 USA
S.M. Faber
Affiliation:
UCO/Lick Observatory, Santa Cruz, CA 95064 USA
A. Dressler
Affiliation:
Carnegie Observatories, Pasadena, CA 91101 USA

Extract

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We present first results of a Hubble Space Telescope imaging and a Palomar and Keck Observatories spectroscopy program of distant, rich galaxy clusters in the form of a “Hubble Atlas” of morphological types at z ≥ 0.75. Two clusters from the compilation of Gunn, Hoessel & Oke (1985) have been studied to date, Cl1322+3027 at z ≈ 0.76 and Cl1603+4313 at z ≈ 0.90.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 455
Copyright
Copyright © Kluwer 1996 

References

Couch, W.J., Ellis, R.S., Sharpies, R.M., & Smail, I. (1994) Ap.J., 430, 121 Google Scholar
Dressler, A., Oemler, A., Butcher, H.R., & Gunn, J.E. (1994) Ap.J., 430, 107 CrossRefGoogle Scholar
Gunn, J.E., Hoessel, J.G., & Oke, J.B. (1985) Ap.J., 306, 30 CrossRefGoogle Scholar
Wirth, G.D., Koo, D.C., & Kron, R.G. (1994), Ap.J. (Lett), 435, L105 Google Scholar