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Globular Cluster Formation in Galaxy Mergers
Published online by Cambridge University Press: 30 March 2016
Abstract
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We present preliminary results of a high resolution simulation of globular cluster formation in a galaxy merger using GADGET (Springel et al. 2001). A barotropic equation of state (Li et al 2003) is implemented to include effects of cooling and heating. After one orbital period, a dozen proto-globular clusters are identified in the tidal tails.
- Type
- JD6: Extragalactic Globular Clusters & Their Host Galaxies
- Information
- Copyright
- Copyright © Astronomical Society of Pacific 2005
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