Hostname: page-component-586b7cd67f-gb8f7 Total loading time: 0 Render date: 2024-11-28T22:53:44.208Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Dolphin, A. E. 2000, PASP, 112, 1383 CrossRefGoogle Scholar
Harris, W. Pritchet, C. J., & McClure, R. D. 1995, ApJ, 441, 120 CrossRefGoogle Scholar
West, M. J., Côte, P., Jones, C., Forman, W., & Marzke, R. O. 1995, AJ, 453, L77 Google Scholar