Palomar-Quest and other modern surveys Some slides borrowed from G. Djorgovsky Arne Henden Director, AAVSO [email protected].
X-ray Properties of Sgr A* Flares A Detailed X-ray View of the Central Parsecs Frederick Baganoff MIT Kavli Institute MIT Mark Bautz George Ricker Zhongxiang.
Los Alamos National Laboratory Adelaide, Australia. December 2006 Gus Sinnis Synoptic TeV Telescopes Results from Milagro Plans for HAWC.
21 November 2002Millimetre Workshop 2002, ATNF Millimetre ATCA Results Vincent Minier School of Physics UNSW.
Charles Hakes Fort Lewis College1. Charles Hakes Fort Lewis College2.
GHz Measurements of anomalous dust emission Richard Davis, Clive Dickinson, Rod Davies, Anthony Banday Paris.
Some 3 body problems Kozai resonance 2 planets in mean motion resonance Lee, M. H. 2004.
A. BELIAS, NESTOR Institute, Pylos, Greece TeVPA 2009, July 13-17, SLAC1 KM3NeT, a deep sea neutrino telescope in the Mediterranean Sea KM3NeT objectives.
Photometry. Measuring Energy Photometry measures the energy from a source using a narrow range of wavelengths. –Visual wavelengths from 400-700 nm –Narrower.
Feedback from Momentum-Driven Winds Eliot Quataert (UC Berkeley) w/ Norm Murray & Todd Thompson NGC 3079 w/ HST.
Neutron Stars 2: Phenomenology Andreas Reisenegger ESO Visiting Scientist Associate Professor, Pontificia Universidad Católica de Chile Chandra x-ray.
Is there a preferred direction in the Universe P. Jain, IIT Kanpur There appear to be several indications of the existence of a preferred direction in.