No CrossRef data available.
Article contents
GEMS: The destiny of Blue Spheroidal Galaxies
Published online by Cambridge University Press: 01 August 2006
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.
One of the key predictions of hierarchical galaxy formation models is that a significant fraction of elliptical galaxies form in late merging events. One of the most important diagnostics of such an assembly is the existence of blue spheroidal galaxies, which have spheroid-dominated morphologies and blue colors indicating recent star formation, as an intermediate step in the evolution of elliptical galaxies.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 102
- Copyright
- Copyright © International Astronomical Union 2007
References
Rix, H., Barden, M., Beckwith, S.V.W., Bell, E.F., Caldwell, J.A.R., Häußler, B., Jahnke, K., Jogee, S., McIntosh, D.H., Meisenheimer, K., Peng, C.Y., Sanchez, S.F., Somerville, R.S., Wisotzki, L., & Wolf, C., 2004, ApJS, 152:163.CrossRefGoogle Scholar