Simulated synchrotron emission from Pulsar Wind Nebulae Delia Volpi Dipartimento di Astronomia e Scienza dello Spazio-Università degli Studi di Firenze-Italia.
An accretion disk-corona model for X-ray spectra of active galactic nuclei Xinwu Cao Shanghai Astronomical Observatory.
THE CANNONBALL MODEL AND SHORT HARD BURSTS Arnon Dar 44 th Rencontre De Moriond, La Thuile, Italy, February 1-8, 2009 Based on work done in collaboration.
The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
Turbulent heating in_galaxy_clusters_brightest_in_x_rays
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Clusters of galaxies The ICM, mass measurements and statistical measures of clustering.
Probing the Neutron Star Equation of State and Synergy with Advanced LIGO and Virgo Cole Miller University of Maryland.
Constraining Cosmography with Cluster Lenses Jean-Paul Kneib Laboratoire d’Astrophysique de Marseille.
The Radio Millisecond Pulsar PSR J1023+0038: A Link to Low-Mass X-Ray Binaries Slavko Bogdanov.
Neutrinos and TeV photons from Soft Gamma Repeater giant flares Neutrino telescopes can be used as TeV detectors for short time scale events using
Entropy in the ICM Institute for Computational Cosmology University of Durham Michael Balogh.
