The Circumstellar Disks and Binary Companions of Be Stars Drew Chojnowski, NMSU Tremendous progress has been made over the past two decades toward understanding Be stars, but a number of key aspects of them remain...
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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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Colloquium Title Emma Dahl, NMSU Abstract textShare this:TweetPrint
Metal Absorption in the Circumgalactic Medium During the Epoch of Reionization Caitlin Doughty, NMSU The characteristics of metal absorption arising from the circumgalactic medium of galaxies have been demonstrated to be related to conditions in...
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Red giants, eclipsing binaries, and asteroseismology. Patrick Gaulme, Max Planck Institute for Solar System ResearchShare this:TweetPrint
The Sunspot Solar Observatory Visitor Center Heidi Sanchez, Sunspot Solar Observatory, NMSUShare this:TweetPrint
Cold Gas and the Evolution of Early-type Galaxies Lisa Young, New Mexico Tech A major theme of galaxy evolution is understanding how today’s Hubble sequence was established — what makes some galaxies red spheroidals and...
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Starless clumps and the earliest phases of high-mass star formation in the Milky Way Brian Svoboda, NRAO Jansky Fellow High-mass stars are key to regulating the interstellar medium, star formation activity, and overall evolution of...
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An Observer’s Examination of the Circumgalactic Medium using Cosmological Simulations Rachel Marra, NMSU A significant aspect to understanding galaxy evolution is having an understanding of the intricacies involving the inflow and outflow of baryons onto...
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A Multi-Wavelength Study of the Evolution of Solar Flares Sean Sellers, NMSU Share this:TweetPrint
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