1 Surviving in academia without selling ones soul A panel discussion moderated by K. Nandakumar Univ. of Alberta.
Department of Physics, South China Univ. of Tech. Properties of Neutron Star and its oscillations 2011.11 collaborators Bao-An Li, William Newton, Plamen.
Observatories and telescopes
Neutron Stars and Black Holes Chapter 14. The preceding chapters have traced the story of stars from their birth as clouds of gas in the interstellar.
Neutron Stars Chapter Twenty- Three. Guiding Questions 1.What led scientists to the idea of a neutron star? 2.What are pulsars, and how were they discovered?
Magnetic aspects of QCD and compact stars T. Tatsumi Department of Physics, Kyoto University I.Introduction and motivation II.Chiral symmetry and spin.
Neutron stars - Chapter 21 1. Neutron stars The remains of cores of some massive stars that have become supernovae. Cores are a degenerate gas of mostly.
Announcements Pick up graded homework (projects, tests still in progress) Transit of Mercury (crossing in front of Sun), this afternoon, roughly noon-5:00.
The “Crab Nebula”: the most famous supernova remnant. distance 2000 pc diameter 3 pc.
Supernovae and Neutron Stars
Death of Stars II
Relativistic Astrophysics: general overview Jean-Pierre Lasota Lecture 1.