Preprint
A comparison of hydrodynamics techniques for modelling collisions between main sequence stars
Abstract
An Eulerian TVD code and a Lagrangian SPH code are used to simulate the
off-axis collision of equal-mass main sequence stars in order to address the
Authors
Trac H; Sills A; Pen U-L
Publication date
May 31, 2006
DOI
10.48550/arxiv.astro-ph/0605753
Preprint server
arXiv