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Lecture 13 Presupernova Models, Core Collapse and Bounce

Lecture 13 Presupernova Models, Core Collapse and Bounce. Density Profiles of Supernova Progenitor Cores. These make the heavy elements. These should be easy to explode. 2D SASI-aided, Neutrino-Driven Explosion?. Poelarends, Herwig, Langer and Heger (2008).

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Supernovae

Supernovae. High Energy Astrophysics emp@mssl.ucl.ac.uk http://www.mssl.ucl.ac.uk/. Introduction. Supernovae occur at the end of the evolutionary history of stars. The star must be at least 2 solar masses: the core at least 1.4 solar masses.

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554 views • 38 slides

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10 solar masses - PowerPoint PPT Presentation

Lecture 13 Presupernova Models, Core Collapse and Bounce

Supernovae