Journal
ASTROPHYSICS AND SPACE SCIENCE
Volume 316, Issue 1-4, Pages 25-30Publisher
SPRINGER
DOI: 10.1007/s10509-007-9560-2
Keywords
stars : evolution; stars : interiors; Sun : evolution
Categories
Ask authors/readers for more resources
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.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available
Share Paper
