Calendar

Sep 21 @ 12:30 pm – 1:30 pm
Pizza Lunch: Drew Chojnowski
APOGEE Be starsShare this:TweetPrint
Dec 4 @ 3:15 pm – 4:15 pm
Colloquium:  Brian Jackson @ BX102
On the Edge: Exoplanets with Orbital Periods Shorter Than a Peter Jackson Movie Brian Jackson, Boise State Univeristy From wispy gas giants to tiny rocky bodies, exoplanets with orbital periods of several days and less...
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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:  Betsy Mills (Host: Moire Prescott) @ BX102
Do star formation laws break in the center of the Galaxy? Betsy Mills, University of Arizona I will review our understanding of molecular gas conditions in the central 500 parsecs of the Milky Way, and summarize recent studies that find that the Galactic center deviates...
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May 12 @ 3:00 pm – 4:00 pm
Colloquium PhD Defense: Kenz Arraki @ Dominici106
Evolution of Dwarf Galaxy Properties in Local Group Environments Kenz Arraki, NMSUShare this:TweetPrint
Sep 9 @ 3:15 pm – 4:15 pm
Colloquium Thesis Proposal: Lauren Kahre @ Biology Annex 102
Extinction mapping with LEGUS Lauren Kahre The study of star formation and galaxy evolution in nearby galaxies depends on obtaining accurate stellar photometry in those galaxies. However, dust in the galaxies hinders our ability to...
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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
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
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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Colloquium: Isak Wold (Host: Moire Prescott) @ BX102
A Faint Flux-Limited LAE Sample at z = 0.3 Isak Wold, UT Austin Observational surveys of Lya emitters (LAEs) have proven to be an efficient method to identify and study large numbers of galaxies over...
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