12 C+ 12 C REACTION AND ASTROPHYSICAL IMPLICATIONS Marco Limongi INAF – Osservatorio Astronomico di Roma, ITALY Institute for the Physics and the Mathematics.
The Modeling of Surface TNR’s on Compact Stars Nova – review X-Ray bursts on NS – first steps.
May 13, 2003Lynn Cominsky - Cosmology A3501 Professor Lynn Cominsky Department of Physics and Astronomy Class web page: lynnc/courses/a350
The Effects of Mass Loss on the Evolution of Chemical Abundances in Fm Stars Mathieu Vick 1,2 Georges Michaud 1 (1)Département de physique, Université.
Class 25 : Active galactic nuclei Discovery of AGN (3C 273). What are AGN? Radio galaxies. AGN and colliding galaxies.
Stars II. Stellar Physics. 1.Overview of the structure of stars Still, First the Sun as an example.
Clicker Question: What is the Helium Flash? A: Explosive onset of Helium fusing to make Carbon B: A flash of light when Helium fissions to Hydrogren C:
The Formation of High Mass Stars Richard I. Klein UC Berkeley, Department of Astronomy and Lawrence Livermore National Laboratory Collaborators Mark Krumholz.
The Phenomenon of Active Galactic Nuclei: an Introduction
Black Holes Escape velocity Event horizon Black hole parameters Falling into a black hole.
Review-Questions (exam next Thursday, April 06 chapter 21-25) Go Mason! Go Through My Notes.
Neutrino oscillations in oxygen-neon-magnesium supernovae