Mar 2 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Gordon MacDonald, NMSU AbstractShare this:TweetPrint
Mar 28 @ 3:15 pm – 4:15 pm Science Hall 109
Seismic Inferences of Gas Giant Planets: Excitation & Interiors Ethan Dederick, NMSU Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars. In...
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Mar 29 @ 4:00 pm – 5:00 pm Gardiner Hall 230
Surprising Impacts of Gravity Waves Jim Fuller, Caltech Gravity waves are low frequency fluid oscillations restored by buoyancy forces in planetary and stellar interiors. Despite their ubiquity, the importance of gravity waves in evolutionary processes...
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Jan 23 @ 3:00 pm – 4:00 pm
Extinction Mapping and Dust-to-Gas Ratios of Nearby Galaxies Lauren Kahre, NMSU We present a study of the dust{to{gas ratios in 31 nearby (D > 10 Mpc) galaxies. Using Hubble Space Telescope broad band WFC3/UVIS UV...
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Nov 15 @ 3:15 pm – 4:15 pm BX102
Using every photon to learn about the physics of solar plasmas Phil Judge, High Altitude Observatory, Boulder CO. The Sun has traditionally been the Rosetta Stone that can overcome the gap in regimes between laboratory...
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Apr 17 @ 3:00 pm – 4:00 pm Online
Evolution of Ionized Interstellar Medium across Cosmic Time Fuyan Bian, European Southern Observatory The ionized interstellar medium (ISM) provides essential information on the star-forming environments, metal enrichment, and underlying ionizing radiation field in galaxies. It...
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