Hostname: page-component-586b7cd67f-rcrh6 Total loading time: 0 Render date: 2024-11-26T01:57:17.137Z Has data issue: false hasContentIssue false

The Origin of High Specific Frequency Globular Cluster Systems

Published online by Cambridge University Press:  25 May 2016

M.G. Lee
Affiliation:
Department of Astronomy, Seoul National University, Seoul 151–742, KOREA
D. Geisler
Affiliation:
KPNO/NOAO, 950 N. Cherry Av., Tucson, AZ 85719 USA

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.

There are known to be several giant elliptical galaxies with high globular cluster specific frequencies, which possess about three or more times the normal number of globular clusters for their luminosity. The origin of high specific frequency globular cluster systems is not yet known.

Type
Mergers & Remnants
Copyright
Copyright © Kluwer 1999