tipa -- 8/12/2010

The Plerionic Supernova Remnant G21.5-0.9 Powered by PSR J1833-1034: New Spectroscopic and Imaging Results Revealed with the Chandra X-ray Observatory

The lithium content of omega Centauri. New clues to the cosmological Li problem from old stars in external galaxies

  • Authors: L. Monaco (1,2), P. Bonifacio (3,4), L. Sbordone (5), S. Villanova (1), E. Pancino (6) ((1) Universidad de ConcepciĆ³n, ConcepciĆ³n, Chile, (2) ESO - European Southern Observatory, (3) GEPI, Observatoire de Paris, Paris, France, (4) Istituto Nazionale di Astrofisica -- Osservatorio Astronomico di Trieste, Trieste, Italy, (5) Max Planck Institut for Astrophysics, Garching, Germany, (6) Istituto Nazionale di Astrofisica -- Osservatorio Astronomico di Bologna, Bologna, Italy)

Gamma-ray Emission from Crushed Clouds in Supernova Remnants

Radio pulsar populations

Constraints on Dark Matter from Colliders

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