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2017 Fall Science Colloquia Webcasts
Wednesday Sep 6, 2017
2017 Fall Science Colloquia
Geronimo Luis Villanueva (Goddard Space Flight Center)
We recently established that Mars lost an ocean’s worth of water, while the Curiosity rover has recently detected organics on the Martian surface and in the atmosphere. If Mars had a rich chemical and diverse past, how much of these biomarkers were l ...
Wednesday Sep 13, 2017
2017 Fall Science Colloquia
Mark Devlin (University of Pennsylvania)
Researchers have been utilizing the measurements of the Cosmic Microwave Background (CMB) for the last several decades to study the birth and evolution of our Universe. I will review the science behind the CMB and describe how we extract cosmologica ...
Wednesday Sep 20, 2017
2017 Fall Science Colloquia
Raffaella Margutti (Northwestern University)
Observations are drawing a complex picture of the latest stages of massive stars evolution and their explosions. In this seminar I concentrate on two among the least understood aspects of stellar evolution, adopting an observational perspective: How ...
Wednesday Oct 4, 2017
2017 Fall Science Colloquia
Megan Donahue  (Michigan State University )
One of the biggest challenges to understanding how galaxies work is decoding the role of the central supermassive black hole. Without feedback from the black hole (“AGN feedback”), galaxy evolution models fail to produce realistic massive galaxies an ...
Wednesday Oct 18, 2017
2017 Fall Science Colloquia
Ortwin Gerhard (Max-Planck-Institut für Extraterrestrische Physik)
The Milky Way has a cylindrically rotating, strongly peanut-shaped bulge which is the inner, three-dimensional part of a longer, flatter bar, as also seen in external galaxies and N-body simulations. Dynamical models based on NIR star counts and kin ...
Wednesday Nov 8, 2017
2017 Fall Science Colloquia
Mariska Kriek (University of California-Berkeley)
No description found.
Wednesday Nov 15, 2017
2017 Fall Science Colloquia
Wendy Freedman (University of Chicago)
Resolving the Tension in the Hubble Constant The accuracy with which we can measure the Hubble constant, Ho has been steadily increasing over the past decade. The direct and traditional means to measure Ho is based on measurement of distances and ...
Wednesday Nov 29, 2017
2017 Fall Science Colloquia
Victoria Kaspi (McGill University)
No description found.
Wednesday Dec 6, 2017
2017 Fall Science Colloquia
Mark Vogelsberger (Massachusetts Institute of Technology)
: In my talk I will describe recent efforts to model the large-scale distribution of galaxies with cosmological hydrodynamics simulations. I will focus on the Illustris simulation, and our new simulation campaign, the IllustrisTNG project. After de ...
Wednesday Dec 13, 2017
2017 Fall Science Colloquia
Gilles Fontaine (University of Montreal)
A few years ago, Charpinet, Fontaine, & Brassard (2009, Nature, 461, 501) developed a new approach to test for solid body rotation (and deviations thereof) in pulsating stars. The method was successfully applied to the prototype of the GW Vir class o ...