Nustar reveals extreme_absortion_in_z_05_type_2_quasars
Current status of numerical relativity Gravitational waves from coalescing compact binaries Masaru Shibata (Yukawa Institute, Kyoto University)
Overview of LIGO 23rd Texas Symposium on Relativistic Astrophysics December 11, 2006 Jay Marx (on behalf of the LIGO Scientific Collaboration) G060579-00-A.
Numerical Relativistic Hydrodynamics José A. Font Departamento de Astronomía y Astrofísica Universidad de Valencia (Spain) Lectures given at the School.
Towards relativistic magneto-rotational core collapse simulations José A. Font Departamento de Astronomía y Astrofísica Universidad de Valencia (Spain)
Key Open Problems in Black Hole Physics and Gravitation Theory Today (A personal perspective!) Pankaj S. Joshi.
Current status of numerical relativity Gravitational waves from coalescing compact binaries
On the gravitational and electrodynamical stability of nuclear matter cores
Improved simulations of relativistic stellar core collapse
Dynamic stability of compact stars. Properties of the neutron star crust. G.S.Bisnovatyi-Kogan Space Research Institute RAN, Moscow Joint Institute of.
Final Fate of a Massive Star Pankaj S. Joshi. The talk is divided in the following main parts: I. INTRODUCTORY II. A STABILITY ANALYSIS: Introducing Small.
Black hole solutions in the N>4 gravity models with higher order curvature corrections and possibilities for their experimental search S.Alexeyev *, N.Popov,