Colloquium Title Sten Hasselquist, NMSU AbstractShare this:TweetPrint
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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Detecting host galaxies of metal absorbers at the end of the dark ages Share this:TweetPrint
Promoting Graduate Student Wellness: A Guide for Faculty and Staff Marie Zubiate, Aggie Health and Wellness Center As graduate students demonstrate signs of emotional and psychological distress, faculty and staff play an important role in...
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Current Efforts in Seismology of the Sun and Stars Share this:TweetPrint
The SPLASH Survey of the Andromeda Galaxy Raja Guhathurkurta, University of California, Santa Cruz Our nearest large spiral galaxy neighbor, the Andromeda galaxy (M31), and its dwarf satellites, offer a panoramic yet detailed view of...
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Solving the Puzzles of the Moon Shun Karato, Yale University After 50 years from the first landing of men on the Moon, about 380 kg of samples were collected by the Apollo mission. Chemical analyses...
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Galaxy Evolution in a Computer Box, or “How to turn a PhD on Theoretical Galaxy Evolution into a Scientific Programming Career with NASA” Jacob Vander Vliet, NASA/SOFIA I graduated from NMSU in 2017 with a...
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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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Simulating Planetesimal Formation in the Kuiper Belt and Beyond Rixin Li, University of Arizona A critical step in planet formation is to build super-km-sized planetesimals in protoplanetary disks. The origin and demographics of planetesimals are...
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