Mar 2 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Gordon MacDonald, NMSU AbstractShare this:TweetPrint
Apr 2 @ 12:30 pm – 1:30 pm AY 119
The quarks in the proton go round and round …Share this:TweetPrint
Apr 6 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Sten Hasselquist, NMSU AbstractShare this:TweetPrint
Sep 6 @ 3:15 pm – 4:15 pm BX102
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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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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Nov 22 @ 3:15 pm – 4:15 pm BX102
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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May 29 @ 2:30 pm – 3:30 pm Online
H-Band Spectroscopy of Exotic, Massive Stars Drew Chojnowski, NMSU We report on spectroscopy of exotic B-type emission line (Be) stars and chemically peculiar (CP) stars in the near-infrared (NIR) H-band, using data provided by the...
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Dec 4 @ 3:00 pm – 4:00 pm BX102
Role of solar Rossby waves in causing space weather on intermediate time-scales Mausumi Dikpati, HAO Forecasting our weather was built on the recognition that global Rossby waves, interacting with mean east-west flow on the Earth’s...
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