Upcoming Events
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Seminar: The Physics of Gas Sloshing in Cool-Core Galaxy ClustersHow simulations of gas sloshing in clusters can explain their formation and evolution, and the implications for the physics of the ICM. February 16, 2012 Pupin 1402
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Big Apple Colloquium: Unifying the Many Faces of Neutron Stars: The High Magnetic Field ConnectionPossible overarching physical theories that can explain the great variety of NS phenomena, and the role of unparalleled magnetic field strengths in these remarkable objects. Feburary 17, 2012 428 Pupin
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Colloquium: Diana ValenciaMIT (TBC) February 22, 2012 1402 Pupin
