Hostname: page-component-84b7d79bbc-g5fl4 Total loading time: 0 Render date: 2024-08-04T02:36:45.243Z Has data issue: false hasContentIssue false
  • English
  • Français

Globular Cluster Formation in Galaxy Mergers

Published online by Cambridge University Press:  30 March 2016

Yuexing Li ,
Mordecai-Mark Mac Low  and
Ralf S. Klessen
Yuexing Li
Affiliation:
Columbia Univ, NY AMNH, NY, USA
Mordecai-Mark Mac Low
Affiliation:
Columbia Univ, NY AMNH, NY, USA
Ralf S. Klessen
Affiliation:
AIP, Potsdam, Germany

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 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
Highlights of Astronomy , Volume 13 , 2005 , pp. 205
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Li, Y., Klessen, R., & Mac Low, M-M, 2003, ApJ, 592, 975 Google Scholar
Springel, V., Yoshida, N. & White, S. 2001, New Astronomy 6, 79 Google Scholar
Springel, V. 2000, MNRAS 312, 859 Google Scholar