ON THE MINIMAL ACCURACY REQUIRED FOR SIMULATING SELF-GRAVITATING SYSTEMS BY MEANS OF DIRECT N-BODY METHODS
The Astrophysical Journal Letters American Astronomical Society 785:1 (2014) l3
A star cluster simulation coupling N-body dynamics and stellar evolution using the Astrophysical Multi-purpose Software Environment (credit: Inti Pelupessy).
Dr Tjarda Boekholt
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