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Past Colloquia

Enhancing our Views of Star Formation in a Galactic Context

Cody Hall, 50 St. George Street

Prof. Erik Rosolowsky, University of Alberta

November 11, 2026
2:00pm - 3:00pm

The conditions in molecular gas must set the initial conditions for star formation.  The rate of star formation and the mass distribution of resulting stars are essential inputs into our models of galaxy evolution.  Thus, we hope to understand the physics that regulates star formation…

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Beadwork as a knowledge translation methodology and tool for reconciliation in astronomy and astrophysics

Cody Hall, 50 St. George Street

Dr. Danielle Lussier (Queen’s University) and Dr. Gregg Wade (Royal Military College of Canada)  

November 04, 2026
2:00pm - 3:00pm

Abstract: In collaboration with the Arthur B. McDonald Canadian Astroparticle Physics Research Institute, Dr. Lussier (Red River Métis legal scholar) and Dr. Wade (settler astrophysicist) are developing beadwork-based artwork as vehicles for astrophysical knowledge translation. Beading works as a science methodology because it is both…

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Galaxies and supermassive black holes at Cosmic Dawn with JWST

Cody Hall, 50 St. George Street

Prof. Rachel Somerville, Rutgers University

October 21, 2026
2:00pm - 3:00pm

Since the launch of the James Webb Space Telescope nearly five years ago, its observations of the early Universe have uncovered multiple new puzzles around how the earliest galaxies and black holes formed and evolved. Apparently, galaxies formed surprisingly early and vigorously, and have ISM…

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CANCELLED

Cody Hall, 50 St. George Street

Prof. Jennifer Bergner

October 14, 2026
2:00pm - 3:00pm

Planets are born from the gas, dust, and ice present within the disks around young stars.  The icy component of the parent disk is profoundly important to the outcomes of planet formation, but prior to JWST there were virtually no observational constraints on ices in…

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How to Make an Astronomer in the Age of AI

Cody Hall, 50 St. George Street

Prof. Michael Reid, University of Toronto

October 07, 2026
2:00pm - 3:00pm

Abstract: Generative AI has caused chaos in higher education, upending old assessment strategies and changing our relationship with our students in uncomfortable ways. As we consider how to respond, it’s an opportunity to revisit some of our deeply held values as educators. We have to…

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Probing Dark Matter with X-ray Telescopes and the International Axion Observatory (IAXO)

Cody Hall, 50 St. George Street

Prof. Kerstin M. Perez

September 30, 2026
2:00pm - 3:00pm

Axions are among the best motivated candidates for dark matter. Their existence would subtly alter the processes within stellar interiors, imprinting characteristic signals in astrophysical observations. Observations with existing X-ray telescopes have already begun to exploit this connection, placing leading constraints on axion dark matter…

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The Beautiful Confusion. The Earliest Galaxies after JWST

Cody Hall, 50 St. George Street

Prof. Andrea Ferrara

September 23, 2026
2:00pm - 3:00pm

One of the major surprises provided by the first months of early Universe observations by JWST has been the detection of a stunning overabundance of luminous, and likely massive, galaxies at redshift z>10. As the first spectroscopic confirmations are  accumulating, it is crucial and timely to…

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The Afterlife of Gas Giants: Tidal Disruption and Subsequent Fate of Stripped Cores on Close-in Orbits

Cody Hall, 50 St. George Street

Prof. Heather Knutson

September 16, 2026
2:00pm - 3:00pm

For decades, models have predicted that gas giant planets that come too close to their host stars will be destroyed, with most of their mass accreted onto the host star.  However, recent work modeling Roche lobe overflow from close-in gas giants now indicates that angular momentum exchange…

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The Seasons of Helium

Cody Hall, 50 St. George Street

Prof. S. R. Kulkarni

September 09, 2026
2:00pm - 3:00pm

SPHEREx, a recently launched astronomy mission, detected a bright 1.083 micron emission feature in the commissioning data. The PI group attributed this feature to the He I 1.0833 micron triplet line. In this seminar I review the physics and aeronomy of this well-known line of…

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“Asteroseismology: from slow to fast rotators and from individual stars to populations”

AB107

Prof. Conny Aerts, KU Leuven, Belgium

May 20, 2026
11:00am - 12:00pm

Abstract: After a brief general introduction into the basic principles of asteroseismology, we consider the various restoring forces and the approximations adopted in the theory of stellar oscillations.  We discuss the corresponding waves and frequency regimes encountered in modern space photometric light curves of various…

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