Simulating Star Cluster Formation within Galactic Disk Models

Details Simulating Star Cluster Formation within Galactic Disk Models Simulating Star Cluster Formation within Galactic Disk Models

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jena.confe..61g&link_type=abstract

"JENAM-2007, "Our non-stable Universe", held 20-25 August 2007 in Yerevan, Armenia. Abstract book, p. 61-61"

Computer Science

Scientific paper

During this presentation we will present our initial results from a series of high-resolution simulations of Milky Way sized disk galaxies using the code ENZO. The simulations are global and three-dimensional, including a treatment of star formation and feedback. Specifically, we will focus the presentation on the formation and evolution of star clusters within these simulations, and compare the simulated stellar clusters to observations.

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