Colloquia Schedule Spring 2014
Colloquia are on Tuesdays (unless otherwise indicated) at 3:30 pm in RLM 15.216B
No talk scheduled. |
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"The Connection between Star Formation and the Cold Interstellar Medium in Nearby Galaxies" University of Arizona host: Shardha Jogee |
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"The Unusual Eclipser of the Young Star J1407: Moon-forming Circumplanetary Disk?" University of Rochester host: TBA |
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"A Calibration of the Stellar-mass Fundamental Plane at
Massachusetts Institute of Technology host: Pawan Kumar |
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Tinsley Visiting Scholar, Interstellar Matter Group "Volatiles in Protoplanetary Disks" Space Telescope Science Institute (STScI) host: Neal Evans |
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DeVaucouleurs Medalist: COLLOQUIUM "Connecting Gas to Stars in Galaxies" University of Cambridge, UK host: Neal Evans |
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DeVaucouleurs Medalist: PUBLIC LECTURE "The Hidden Universe Revealed" University of Cambridge, UK host: Neal Evans |
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"The Seeds of Massive Galaxies" University of Edinburgh host: Shardha Jogee |
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"Our Galactic Supermassive Black Hole Sgr A*: The Ideal Testbed for Theories of Accretion and Black Hole Life Cycles" University of Amsterdam host: Pawan Kumar |
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Spring Break: 10-14 March: No talk scheduled. |
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"Rest-frame Optical Spectra: A Window into Galaxy Formation at z~2" University of California, Los Angeles host: Steve Finkelstein |
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Tinsley Visiting Scholar, Stars Group "Hunting the First Generations of Stars and Galaxies" Massachusetts Institute of Technology host: Fritz Benedict |
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"Shadows of Their Future Selves: Accretion and Obscuration in Young Stellar Objects" Lowell Observatory host: Adam Kraus |
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"Head in the Clouds: Decoding the Spectral Features Produced by Brown Dwarf and Exoplanent Atmospheres" Hunter College/AMNH host: Adam Kraus |
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PhD Defense Presentation "Measuring Dark Matter Profiles Non-Parametrically in Dwarf Spheroidal Galaxies" The Milky Way's Dwarf Spheroidal galaxies (dSphs) are
some of the smallest galaxies in the Universe, and yet
they have some of the highest concentrations of dark
matter. These nearby galaxies have been extensively
studied with dynamical models hoping to measure the
distribution of dark matter in them. Unfortunately,
past models have relied on overly restrictive assumptions,
or have been crippled by degeneracies and lacked predictive
power. In this dissertation talk, I introduce a significant
improvement into the field of dynamical modeling, and I
use it to make robust and detailed measurements of the dark
matter density profiles in five dSphs: Carina, Draco,
Fornax, Sculptor, and Sextans. By relaxing assumptions
about the shape of these galaxies' dark matter profiles,
I am able to recover a variety of profile types. Some of
these fit with expectations from theoretical simulations,
others match profiles observed in other galaxies, and still
others were found to have completely unexpected shapes.
I compare my findings with results from hydrodynamical
simulations to speculate on a relationship between profile
shape and baryon content.
University of Texas at Austin |
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"Hunting the First Galaxies with Gravitational Lensing" Space Telescope Science Institute (STScI) host: Steve Finkelstein |
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Tinsley Visiting Professor "Adventures in Cosmic Star Formation" National Optical Astronomy Observatory (NOAO) host: TBA |
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Tinsley Visiting Scholar, Exgal Group "MaNGA: Mapping Nearby Galaxies at Apache Point Observatory An IFU Survey of 10,000 Galaxies" University of Tokyo, IPMU host: Niv Drory |
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Tinsley Visiting Scholar, Planets Group "Extrasolar Planets with Small Telescopes" Princeton University host: Mike Endl |
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No talk scheduled. |
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"Stark Broadening of Hydrogen Spectral Lines in Plasmas: Advanced Theories, Benchmark Experiments, Astrophysical Applications" Auburn University host: Don Winget |
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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