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A Comparative Study of Globular Cluster Systems in UGC 9799 and NGC 1129

Published online by Cambridge University Press:  03 August 2017

Myung Gyoon Lee ,
Eunhyeuk Kim ,
Doug Geisler ,
Terry Bridges  and
Keith Ashman
Myung Gyoon Lee
Affiliation:
Astronomy Program, SEES, Seoul National University, Seoul, 151–742, Korea
Eunhyeuk Kim
Affiliation:
Astronomy Program, SEES, Seoul National University, Seoul, 151–742, Korea
Doug Geisler
Affiliation:
Departamento de Física, Grupo de Astronomía, Universidad de Concepción, Casilla 160-C, Concepción, Chile
Terry Bridges
Affiliation:
Anglo-Australian Observatory, P. O. Box 296, Epping, NSW 1710, Australia
Keith Ashman
Affiliation:
Department of Physic and Astronomy, University of Kansas, Lawrence, KS 66045–2151, USA

Abstract

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We present a preliminary analysis of HST-WFPC2 observations of globular cluster systems in the two brightest galaxies, UGC 9799 (cD) and NGC 1129 (non-cD), located in the center of rich clusters.

Type
Part 2. Globular Cluster Systems of Distant Galaxies
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 330 - 332
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

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