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SPH Calculations of Collisions Between Main-Sequence Stars

Published online by Cambridge University Press:  25 May 2016

Frederic A. Rasio
Frederic A. Rasio*
Affiliation:
Department of Physics, M.I.T. 6-201, Cambridge, MA 02139, USA

Abstract

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The hydrodynamics of collisions and mergers of main-sequence stars is discussed in the light of recent 3-D calculations using the smoothed particle hydrodynamics (SPH) method. Theoretical models for the formation of blue stragglers are reviewed in the context of recent comparisons between the observed properties of blue stragglers in dense globular clusters and the predictions of those models.

Type
August 25: X Ray and Compact Objects in Globular Clusters
Information
Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 253 - 262
Copyright
Copyright © Kluwer 1996 

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