Colloquia Schedule Fall 2011
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
Not your Parents' M Dwarfs: Probing the Milky Way with its Smallest Constituents (Cancelled due to Hurricane Irene: to be rescheduled) Boston University host: Colette Salyk |
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Maxwell, Einstein, and Their Impossibilities Center for Nonlinear Dynamics & Dept. of Physics, University of Texas at Austin hosts: Paul Shapiro & Tanja Rindler-Daller |
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Dark Matter, Dwarf Galaxies, and Massive Failures in the Halo of the Milky Way University of California, Irvine host: TBD |
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Black Hole Scaling Relations University of Michigan host: Karl Gebhardt |
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The Quest for the Dynamical Signature of Close Supermassive Binary Black Holes Pennsylvania State University host: Julie Comerford |
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What is a Galaxy? Haverford College host: TBD |
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No talk scheduled, to avoid conflict with Frank N. Bash Symposium |
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Status update on the James Webb Space Telescope project NASA Goddard Space Flight Center host: TBD |
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GAMA: from Little Blue Fuzzies to Massive Red Monsters and Beyond Swinburne University host: Karl Gebhardt |
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Casting Shadows on the Standard Interstellar Medium Paradigm with GALFA-HI Columbia University host: Sarah Tuttle |
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Beatrice M. Tinsley Visiting Scholar The Origins of Planetary Systems - Constraints from Protoplanetary Disks University of Arizona host: John Lacy |
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No talk scheduled. |
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No talk scheduled. |
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Stellar Forensics with Explosions: Supernovae, Gamma-Ray Bursts, and their Environments Long-duration gamma-ray bursts (GRBs) and Type Ib/c Supernovae (SN
Ib/c) are nature's most magnificent explosions from massive
stars. While GRBs launch relativistic jets, SN Ib/c are core-collapse
explosions whose progenitors have been stripped of their hydrogen and
helium envelopes. Yet for over a decade, one of the key outstanding
questions is what conditions lead to each kind of explosion in massive
stripped stars. Determining the fates of massive stars is not only a
vibrant topic in itself, but also impacts using GRBs as star formation
indicators over distances up to 13 billion light-years and for mapping
the chemical enrichment history of the universe. New York University, Center for Cosmology and Particle Physics host: Sarah Tuttle |
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HETDEX Special Colloquium Astrophotonics and Space Photonics: A New Era of Instrumentation University of Sydney, School of Physics host: Sarah Tuttle |
Visitors to the Department of Astronomy can find detailed information and maps on our Visiting Austin Page.
Please report omissions/corrections to: G. Orris at argus@astro.as.utexas.edu.
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