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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Clues to Globular Cluster Formation David Nataf, Johns Hopkins University Globular clusters are now well-established to host “Second-generation” stars, which show anomalous abundances in some or all of He, C, N, O, Na, Al, Mg,...
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Safe Zone Training Dr. Zooey Sophia Pook, NMSU The SafeZone Training was established to educate and train students, faculty, and staff on how to provide safe and affirming support to members of the gay, lesbian, bisexual, transgender, and questioning...
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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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Charting the Outer Reaches of Exoplanetary Systems: Wide-Separation Giant Planet Demographics with Direct Imaging Eric Nielsen, Kavli Institute for Particle Astrophysics and Cosmology, Stanford University Over the past decade, the combination of advances in adaptive...
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