The Role of Radiation in Common Envelope Evolution
DOI:
https://doi.org/10.17307/wsc.v1i1.346Schlagworte:
Hydrodynamics, Binaries, Numerical Methods, RadiationAbstract
The common envelope phase in binary star systems is simulated using the 3-D moving-mesh hydrodynamic code MANGA. The radiation hydrodynamics module in MANGA is modified using a sub-cycling algorithm to skip unnecessary calculations. The sub-cycling as well as other optimizations reduce computation time by a factor of 3. The generation of appropriate initial conditions for radiation hydrodynamic simulations is discussed.Literaturhinweise
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