Supernovae are the most energetic events in the evolution of stars. They also are relatively rare events, with the last one observed in our Milky Way Galaxy dating back nearly 400 years. Therefore, the event of Supernova 1987A that occured in February of 1987 in the Large Magellenic Cloud, at a distance of 160,000 light-years, was hailed as a major astronomical event and created much activity both in observing the event and in explaining it theoretically. Woosley works at the cutting edge of modelling supernova outbursts and the evolution of the precursor stars leading up to the explosion, using hydrodynamic numerical modeling and extensive nuclear reaction networks. The main focus of the current proposal is to model Supernova 1987A and its precursor star.

Agency
National Science Foundation (NSF)
Institute
Division of Astronomical Sciences (AST)
Application #
8813649
Program Officer
Edward G. Schmidt
Project Start
Project End
Budget Start
1988-11-01
Budget End
1992-04-30
Support Year
Fiscal Year
1988
Total Cost
$318,860
Indirect Cost
Name
University of California Santa Cruz
Department
Type
DUNS #
City
Santa Cruz
State
CA
Country
United States
Zip Code
95064