No CrossRef data available.
Article contents
The Connection Between dE and dI Galaxies
Published online by Cambridge University Press: 12 April 2016
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 combine specific globular cluster frequencies (SN) with newly measured surface brightness profiles to identify dEs that may be stripped dIs. Luminous dEs generally have higher surface brightnesses and steep central light profiles. Conversely, fainter dEs have low surface brightnesses and flatter central light profiles. The most likely candidates for stripped dIs have low SN and low central surface brightnesses.
- Type
- The evolution of Low Surface Brightness galaxies
- Information
- International Astronomical Union Colloquium , Volume 171: The Low Surface Brightness Universe , 1999 , pp. 271 - 273
- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
Miller, B.W., Lotz, J., Ferguson, H.C., Stiavelli, M., & Whitmore, B.C.
1998, ApJ, in pressGoogle Scholar
You have
Access