Calendar

Dec 4 @ 7:00 pm – 9:00 pm
Tombaugh Observatory Open House @ Tombaugh Observatory
Open to the public. Faculty member: James Murphy Graduate Students: Jacob Vander Vliet, Kyle Uckert    Share this:TweetPrint
Dec 7 @ 12:30 pm – 1:30 pm
Pizza Lunch: Chunming Zhu
TBDShare this:TweetPrint
Colloquium:  Gail Zasowski  (Host: Drew Chojnowski) @ 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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Colloquium Thesis Proposal:  Sten Hasselquist @ Hardman/Jacobs 225
Title:  TBD Sten Hasselquist   Share this:TweetPrint
May 31 @ 3:00 pm – 4:00 pm
Colloquium PhD Defense: Diane Feuillet @ Dominici106
Ages and Abundance of Local Stellar Populations Diane Feuillet, NMSUShare this:TweetPrint
Sep 19 @ 12:30 pm – 1:30 pm
Pizza Lunch: Reta Beebe @ AY 119
Title: JUNO Reta Beebe A .pdf of the talk can be found here.    Share this:TweetPrint
Colloquium: Amy Simon (Host: Nancy Chanover) @ 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
Pizza Lunch: Drew Chojnowski @ AY 119
Title: H-band Spectral Variability of Classical Be Stars Drew Chojnowski  Share this:TweetPrint
Nov 18 @ 3:15 pm – 4:15 pm
Colloquium: Karen Olsen @ Biology Annex 102
Simulations of the interstellar medium at high redshift: What does [CII] trace? Dr. Karen Olsen, Arizona State University We are in an exciting era were simulations on large, cosmological scales meet modeling of the interstellar medium (ISM)...
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Feb 24 @ 3:15 pm – 4:15 pm
Colloquium: Thomas Rivinius
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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