The Effects of Changes in Reaction Rates on Simulations of Nova Explosions

Classical novae participate in the cycle of Galactic chemical evolution in which grains and metal enriched gas in their ejecta, supplementing those of supernovae, AGB stars, and Wolf-Rayet stars, are a source of heavy elements for the ISM. Once in the diffuse gas, this material is mixed with the exi...

Ausführliche Beschreibung

Bibliographische Detailangaben

Hauptverfasser:	Starrfield, Sumner, Iliadis, Christian, Hix, William Raphael, Timmes, Francis X., Sparks, Warren M.
Format:	Tagungsbericht
Sprache:	eng
Schlagworte:	CARBON CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS EXPLOSIONS GASES HYDROCARBONS NOVAE NUCLEAR PHYSICS NUCLEAR PHYSICS AND RADIATION PHYSICS NUCLEAR REACTIONS REACTION KINETICS SILICATES STARS SUPERNOVAE WOLF-RAYET STARS
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