Stuttgart 2012 – scientific programme
Parts | Days | Selection | Search | Updates | Downloads | Help
EP: Fachverband Extraterrestrische Physik
EP 17: Astrophysik II
EP 17.4: Talk
Thursday, March 15, 2012, 15:30–15:45, V55.02
The morphology of young supernova remnants — •Sonja Boyer, Dominik Elsässer, and Karl Mannheim — Institut für Theoretische Physik und Astrophysik, Universität Würzburg
Core-collapse supernovae are among the candidate sites suggested for heavy element nucleosynthesis. Metallicity evolution of the Galaxy however seems to mandate that explosive nucleosynthesis of iron-group and above elements cannot take place in all core-collapses. We survey archival X-ray data with the aim to probe correlations between asymmetries of supernova remnants - potentially due to highly asymmetric explosions - and heavy element production.