Mar 28 @ 3:15 pm – 4:15 pm Science Hall 109
Seismic Inferences of Gas Giant Planets: Excitation & Interiors Ethan Dederick, NMSU Seismology has been the premier tool of study for understanding the interior structure of the Earth, the Sun, and even other stars. In...
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Oct 5 @ 3:15 pm – 4:15 pm BX102
Clues to Globular Cluster Formation David Nataf, Johns Hopkins University Globular clusters are now well-established to host “Second-generation” stars, which show anomalous abundances in some or all of He, C, N, O, Na, Al, Mg,...
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Oct 19 @ 3:15 pm – 4:15 pm BX102
Understanding How Galaxies Reionized the Universe  Sanchayeeta Borthakur, Arizona State University Identifying the population of galaxies that was responsible for the reionization of the universe is a long-standing quest in astronomy. While young stars can...
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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
Aug 30 @ 3:15 pm – 4:15 pm BX102
Cold Gas and the Evolution of Early-type Galaxies Lisa Young, New Mexico Tech A major theme of galaxy evolution is understanding how today’s Hubble sequence was established — what makes some galaxies red spheroidals and...
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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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Dec 6 @ 3:15 pm – 4:15 pm BX102
Revealing reionization with the thermal history of the intergalactic medium Elisa Boera, SISSA Trieste During hydrogen reionization the UV radiation from the first luminous sources injected vast amount of energy into the intergalactic medium, photo-heating...
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Feb 1 @ 12:30 pm – 1:15 pm Online
Pokemon Planet James McAteer, NMSU Why is this picture correct? And what does that have to do with Pikachu?  Share this:TweetPrint
Feb 12 @ 9:00 am – 10:00 am BX102
The Aditya-L1 mission: ISRO’s first solar observatory in space Durgesh Tripathi, Inter-University Centre for Astronomy and Astrophysics Abstract: Aditya-L1 is the first space mission of ISRO dedicated to solar observation. With seven payloads on boards,...
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Feb 19 @ 9:00 am – 10:00 am BX102
Small Statistics No More: a suite of galaxy simulations to interpret observations Alyson Brooks, Rutgers University The past decade has seen tremendous progress in simulating realistic dwarf galaxies.  Despite the hype, not all dwarfs are...
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Feb 26 @ 3:00 pm – 4:00 pm BX102
Characteristics of Gaseous Counter-rotating Galaxies and their Role in Galaxy Evolution Minje Beom, NMSU A counter-rotating galaxy is a galaxy having one or more component with opposite angular momentum to the main stellar disk. Absent...
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Mar 5 @ 3:00 pm – 4:00 pm BX102
Colloquium Title Jodi Berdis, NMSU Abstract text Share this:TweetPrint
Mar 12 @ 3:00 pm – 4:00 pm BX102
Constraining Galaxy Formation and Baryonic Effects on LSS with Observations of the Thermal and Kinetic Sunyaev-Zeldovich Effects Nicolas Battaglia, Cornell University A new window into the growth and evolution of large-scale structure has opened up...
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Mar 19 @ 3:00 pm – 4:00 pm BX102
The view of early massive galaxies in the run up to JWST Christina Williams, University of Arizona Our most powerful telescopes have glimpsed galaxies in their early growth phase only a few billion years after...
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Mar 26 @ 9:00 am – 10:00 am BX102
Unveiling the physics of gaseous halos through X-ray spectroscopy Aurora Simionescu, Netherlands Institute for Space Research As bright X-ray emitters, the cores of clusters of galaxies have been studied for over 50 years, with many...
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Apr 2 @ 3:00 pm – 4:00 pm BX102
Colloquium Title Colloquium Speaker Name, Affiliation Abstract textShare this:TweetPrint
Apr 7 @ 12:00 pm – 1:00 pm BX102
Implications of z>5 metal absorption for the sources and progression of hydrogen reionization Caitlin Doughty, NMSU The epoch of reionization occurred over 12 billion years ago, and saw the neutral hydrogen in the intergalactic medium...
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Apr 9 @ 3:00 pm – 4:00 pm Remote via Zoom
A Bayesian Approach to Helioseismic Inversions of Subsurface Solar Flows Alec Herczeg, NMSU Helioseismology is a branch of solar physics dedicated to the understanding of the subsurface flows within the Sun. To accomplish this goal,...
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Apr 16 @ 9:00 am – 10:00 am BX102
Colloquium Title : Sun Space Art Prof. Helen Mason, DAMTP University of Cambridge The talk would cover Solar eclipse and communicating solar physics by the medium of arts and crafts. (Details to follow) Share...
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Apr 16 @ 3:00 pm – 4:00 pm
A Galactic Self-Portrait: 3D density map and integrated properties of the Milky Way Julie Imig, NMSU The Milky Way Galaxy, our home, is the ideal laboratory for studying galaxy formation and evolution. The star formation...
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Apr 23 @ 3:00 pm – 4:00 pm BX102
Spatially Resolved Galaxy Interactions Jorge Moreno, Pomona College The focus of this talk is to address the spatial structure and evolution of star formation and the interstellar medium ISM in interacting galaxies. We use an...
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Apr 30 @ 3:00 pm – 4:15 pm Online
Title Laurel Farris, NMSU Share this:TweetPrint
Apr 30 @ 3:00 pm – 4:00 pm BX102
Colloquium Title Colloquium Speaker Name, Affiliation Abstract textShare this:TweetPrint
May 7 @ 9:00 am – 10:00 am BX102
Colloquium Title Colloquium Speaker Name, Affiliation Abstract text Share this:TweetPrint