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Numerical simulations of elliptical galaxies

Published online by Cambridge University Press:  21 October 2010

Chiaki Kobayashi
Chiaki Kobayashi*
Affiliation:
The Australian National University, Mt. Stromlo Observatory, Cotter Rd., Weston ACT 2611, email: [email protected]
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For the formation of elliptical galaxies, two scenarios, monolithic collapse vs. major merger, have been debated. We simulate the formation and chemodynamical evolution of 128 Es from the CDM initial fluctuations, using the GRAPE-SPH code that include star formation, supernovae feedback, and chemical enrichment. In our CDM-based scenario, galaxies form through the successive merging of subgalaxies with various masses.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 282
Copyright
Copyright © International Astronomical Union 2010