Tiziana Di Matteo et al- Direct Cosmological Simulations of the Growth of Black Holes and Galaxies
Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core becomes degenerate Core collapses;
Slide 1 Calculate the net force acting on a particle Mass transfer in a binary system.
Chemical evolution of Super-AGB stars The Giant Branches Lorentz Center, May 2009 Enrique García-Berro 1,2 1 Universitat Politècnica de Catalunya 2 Institut.
1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
The Modeling of Surface TNR’s on Compact Stars Nova – review X-Ray bursts on NS – first steps.
Additional Image Set for 2007 Science Olympiad
Degenerate Matter and White Dwarfs. Summary of Post-Main-Sequence Evolution of Sun-Like Stars M < 4 M sun Fusion stops at formation of C,O core. C,O core.
RS Oph : Unstable Disk Model
Summary of Post-Main-Sequence Evolution of Sun-Like Stars
Future Directions in High Resolution Astronomy A Celebration of the 10th Anniversary of the VLBA
NEWS FROM GALACTIC XRBs „Cloudy” weather in SgXRBs The mystery of the missing population of Be/BH XRBs Spins of compact objects in XRBs.
