Sep 28 @ 3:15 pm – 4:15 pm BX102
Spatial Curvature, Dark Energy Dynamics, Neither, or Both? Bharat Ratra, Kansas State University Experiments and observations over the two last decades have persuaded cosmologists that (as yet undetected) dark energy is by far the main...
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Jan 23 @ 3:00 pm – 4:00 pm
Extinction Mapping and Dust-to-Gas Ratios of Nearby Galaxies Lauren Kahre, NMSU We present a study of the dust{to{gas ratios in 31 nearby (D > 10 Mpc) galaxies. Using Hubble Space Telescope broad band WFC3/UVIS UV...
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Jan 25 @ 11:30 am – 12:30 pm AY 119
How to Write A Competitive Prize Postdoc Application Dale Frail, NRAOShare this:TweetPrint
Jan 25 @ 3:15 pm – 4:15 pm BX102
Multi-Messenger EM-GW Astronomy: The View from the Radio End of the EM Spectrum Dale Frail, NRAO Abstract: With the discovery of gravitational waves and electromagnetic radiation from the binary neutron star merger GW170817, the era...
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Feb 20 @ 3:15 pm – 4:15 pm Domenici Hall
The AAVSO Program: A Resource for Variable Star Research Stella Kafka, AAVSO The AAVSO was formed in 1911 as a group of US-based amateur observers obtaining data in support of professional astronomy projects. Now, it...
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Feb 22 @ 12:15 pm – 1:15 pm AY 119
Title Takashi Sekii, National Astronomical Observatory of Japan AbstractShare this:TweetPrint
Mar 4 @ 12:30 pm – 1:30 pm AY 119
Ultraviolet Observations of Galaxies Mark Rutkowski, Minnesota State Univeristy Ultraviolet observations are essential for answering fundamental questions regarding the role and impact of galaxies in universe. I’ll discuss a number of past, ongoing, and future...
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Mar 5 @ 7:30 pm – 8:45 pm ASNMSU Center for the Arts
Dr. Janna Levin Barnard College   Info here:    Share this:TweetPrint
Mar 19 @ 7:30 pm – 8:30 pm Domenici Hall 109
Our Future in Space: The Moon and Beyond Jack Burns, University of Colorado Boulder Why do we explore space? How do we explore space? Where should we explore? What are the tools for space exploration?...
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Apr 5 @ 3:15 pm – 4:15 pm BX102
A Masing BAaDE’s Window Ylva Pihlström, University of New Mexico Evolved, intermediate mass stars are tracers of an intermediate age stellar population. Due to high mass-loss rates, they harbor circumstellar envelopes, in which different types...
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Apr 17 @ 3:15 pm – 4:15 pm AY 119
Searching for diffuse radio emission in merging galaxy clusters with LOFAR Amanda Wilber, Universität Hamburg Galaxy cluster mergers are powerful drivers of turbulence and shocks, which can accelerate cosmic-ray electrons within the magnetic field of...
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Apr 22 @ 12:30 pm – 1:30 pm AY 119
ASTR 598Share this:TweetPrint
Apr 26 @ 3:15 pm – 4:15 pm BX102
The Role of Ecology in Star and Planet Formation Megan Reiter, Royal Observatory Edinburgh Understanding how feedback regulates star and planet formation is one of the outstanding unsolved problems in astrophysics. Stellar feedback affects all...
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Apr 29 @ 12:30 pm – 1:30 pm AY 119
ASTR 598Share 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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