Computational Astrophysics of Stars

Details Computational Astrophysics of Stars Computational Astrophysics of Stars

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aas...184.5003a&link_type=abstract

American Astronomical Society, 184th AAS Meeting, #50.03; Bulletin of the American Astronomical Society, Vol. 26, p.943

Physics

Scientific paper

The incorporation of realistic microphysics with modern hydrodynamical methods gives new opportunities to solve recalcitrant problems of stellar evolution, especially those involving rapid change. Examples to illustrate such progress will include (1) convective oxygen burning in massive stars, (2) flames and detonations in Type I supernovae, (3) Novae, (4) Accretion, (5) Instabilities driving mixing, and (6) Explosive nucleosynthesis and the mass cut in Type II supernovae. Future prospects for improvement from hardware, algorithms, and better understanding will be discussed.

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