Crab Nebula
Cosmic Fireworks: Supernova Explosions
Rotation and Accretion Powered Pulsars - Pranab Ghosh
Current Radio Sources Crystal Rattazzi, Becky Harris, Shawn Peters, Chuck Fultz, Matt Storey, Zach Brown.
Boom! Within 0.25s core is neutrons with radius 20 km and super-nuclear density Very little light can escape, energy carried off by neutrinos. Power emitted.
The Discovery of the Neutron Star The Neutron Predicted by Ernest Rutherford in 1920 Experimentally discovered by James Chadwick in 1932.
Neutron Stars and Black Holes Why do we expect neutron stars exist? How do we know neutron stars exist? What theoretical arguments predict the existence.
25 ii 2011NASM1 Exploring the Crab Nebula with the Hubble, Chandra and Fermi Space Telescopes Roger Blandford KIPAC Stanford.
Preliminary results of giant pulse investigations from Crab pulsar with Radioastron. Rudnitskiy A.G., Popov M.V., Soglasnov V.A. 12 th EVN SYMPOSIUM Cagliari,
(Recalling the Death of a High-Mass Star…). Neutron stars, although they have 1–3 solar masses, are so dense that they are very small. This image.
SWAN : Sky Watch Array Network ---- A Strategic Initiative --desh Raman Research Institute, Bangalore, India Pre-ASI workshop on Transients @NCRA, Pune.
Jonathan Gair Graduate Seminar, St.Catharine’s College, 28 th November 2005 The Black Hole Symphony – listening to the Universe with gravitational waves.
