We summarize the main physical assumptions and numerical procedures adopted by the FRANEC code to compute stellar models in all the evolutionary phases at hydrostatic and thermal equilibrium. An application to the Standard Solar Model is also briefly presented.
The FRANEC stellar evolutionary code
DEGL'INNOCENTI, SCILLA;PRADA MORONI, PIER GIORGIO;
2008-01-01
Abstract
We summarize the main physical assumptions and numerical procedures adopted by the FRANEC code to compute stellar models in all the evolutionary phases at hydrostatic and thermal equilibrium. An application to the Standard Solar Model is also briefly presented.File in questo prodotto:
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