Hostname: page-component-788cddb947-jbjwg Total loading time: 0 Render date: 2024-10-14T07:49:12.419Z Has data issue: false hasContentIssue false
  • English
  • Français

Mass Distributions of Galaxies by Globular Cluster Systems

Published online by Cambridge University Press:  19 July 2016

Kazutomo Takayanagi
Kazutomo Takayanagi*
Affiliation:
Ryukoku University and Kyoto University

Extract

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.

Density curves of polytrope index 5 were fitted to the surface density distributions of 26 globular cluster systems. Though we have shown only two of them in Fig. 1, the remaining systems resemble the above cases. No differences exist between elliptical and spiral galaxies.

Type
Chapter IX. Poster Papers on Cluster Systems in Distant Galaxies. Deep Photometry and CM Diagrams
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 639 - 640
Copyright
Copyright © Kluwer 1988