Mysteries of the oscillations of gas accreting onto black holes, neutron stars, and white dwarfs
Dr. Wagoner will survey the QPOs (quasi-periodic oscillations) seen in the luminosity fluctuation power spectra of compact objects accreting from a binary companion star. There is little understanding of the different frequency relationships in these systems. Dr. Wagoner will focus on the theory and observations of black holes, and compare the predictions of their spin via diskoseismolgy with those from two other methods.
Speaker: Bob Wagoner, Stanford
Wednesday, 02/15/12
Contact:
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SETI Institute Colloquium Series
189 Bernardo Ave
Mountain View, CA 94043
USA
Mountain View, CA 94043
USA
Phone: 650.961.6633
Website: Click to Visit
