Calendar

Sep 21 @ 12:30 pm – 1:30 pm
APOGEE Be starsShare this:TweetPrint
Mar 4 @ 3:15 pm – 4:15 pm BX102
New Tools for Galactic Archaeology from the Milky Way Gail Zasowski, John Hopkins University One of the critical components for understanding galaxy evolution is understanding the Milky Way Galaxy itself — its detailed structure and...
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Apr 20 @ 1:00 pm – 2:00 pm Hardman/Jacobs 225
Title:  TBD Sten Hasselquist   Share this:TweetPrint
May 31 @ 3:00 pm – 4:00 pm Dominici106
Ages and Abundance of Local Stellar Populations Diane Feuillet, NMSUShare this:TweetPrint
Sep 20 @ 3:00 pm – 4:00 pm Science Hall 310
Utilizing Planetary Oscillations to Constrain the Interior Structure of the Jovian Planets Ethan Dederick Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars....
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Nov 11 @ 3:15 pm – 4:15 pm Biology Annex 102
Outer Planets Update Dr. Amy Simon, NASA The Hubble Outer Planet Atmospheres Legacy (OPAL) program is a yearly program for observing each of the outer planets over two full rotations. Observations began with Uranus in...
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Nov 14 @ 12:30 pm – 1:30 pm AY 119
Title: H-band Spectral Variability of Classical Be Stars Drew Chojnowski  Share this:TweetPrint
Feb 24 @ 3:15 pm – 4:15 pm
Our Current Understanding of Classical Be Stars Dr. Thomas Rivinius, Chile, ESO Paranal I will introduce Be stars as B-type stars with gaseous disks in Keplerian rotation. These disks form by mass ejection from the star itself...
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Mar 6 @ 12:30 pm – 1:30 pm
JIVE/JOVIAL, a network for Jupiter’s seismology and atmosphere dynamics F.X. Schmider, Observatoire de la Cote d’AzurShare this:TweetPrint
Apr 7 @ 3:15 pm – 4:15 pm BX102
The growth of Earth’s inner core: a new technique to constrain seismic properties in its outermost layers Dr. Lauren Waszek, Department of Physics, NMSU The inner core displays a hemispherical difference in seismic velocity, attenuation,...
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Apr 6 @ 3:15 pm – 4:15 pm BX102
Colloquium Title Sten Hasselquist, NMSU AbstractShare this:TweetPrint