Seminar Date:
Friday, May 9th, 2014
Special Time:
3:15-4:15
Speaker:
Dr. Arielle Phillips
Research Faculty
Notre Dame Department of Physics & Astronomy
Title:
In the Neighborhood:
Of Galaxies, Nobel Laureates and Gummy Worms
Abstract:
We will journey from the cosmic web that envelops galaxies as they form, to a network of scientists that made a Nobel Prize winning discovery, and finally to the sinuous lengths of gummy worms to explore what they reveal about the very nature of light.
The formation, evolution, and chemical composition of galaxies are influenced by their interactions with the material immediately around them, or circumgalactic medium. Beyond this lies the intergalactic medium (IGM) which is composed of extensive clusters, filaments, and sheets of galaxies with vast empty expanses (voids) between them. We use a modified computer vision algorithm to identify and extract structures in large-scale simulations (clusters, filaments, voids.) Our understanding of the physical properties and extent of IGM structures leads to a clearer interpretation of their role in the evolution of galaxies and the surrounding circumgalactic medium.
Artistic representations of science tend to focus on the individual scientist with a marked preference for the single genius. The discovery of the accelerating universe, which involved two international teams, totaling fifty scientists, demonstrates how collaboration has become a central component of the scientific process. The High Z Project will give the public an insider’s perspective into the unusually non-hierarchical nature of the collaboration between the twenty scientists on the High Z Supernovae Search Team. Through a hybrid installation and performance, the audience will gain behind the scenes access to the the scientific quest, the collaboration, and the personal journeys behind the discovery of the accelerating universe.
Finally, I will touch on the extensive outreach efforts of physicists at Notre Dame and reveal how we use gummy worms to introduce children to spectra.
Time: 4:15-5:15pm
Location: Large Conference Room
All Adler staff are welcome!
Thursday, May 1, 2014
Tuesday, February 18, 2014
Dislodged & Ionized: Gaseous Structures of the Magellanic Clouds
Seminar Date:
Friday, February 28, 2014
Special Time:
3:15-4:15
Speaker:
Dr. Kat Barger
NSF Postdoctoral Fellow
University of Notre Dame
Title:
Dislodged & Ionized: Gaseous Structures of the Magellanic Clouds
Abstract:
Galaxy evolution is governed by an intricate ballet of gaseous inflows and outflows and galaxy interactions. The nearby Magellanic Clouds provides an advantageous opportunity to study these processes in detail. In this talk, we will explore the gas flows associated with these galaxies through H-alpha emission- and UV absorption-line observations. Galaxy interactions have greatly disturbed the Magellanic Clouds and have tidally displaced massive amounts of gas from these galaxies. These interactions have also triggered intense star formation throughout their disks; we provide compelling evidence that this elevated star formation drives even more material from these galaxies in wide spread, feedback driven winds. Through these observations, we determine the properties of these gas flows and explore their fates. We find that over a billion solar masses of gas neutral and ionized gas surrounds these galaxies. Much of this dislodged gas is transferring between the Magellanic Clouds and the Milky Way, depleting and replenishing their star formation gas reservoir respectively.
Friday, February 28, 2014
Special Time:
3:15-4:15
Speaker:
Dr. Kat Barger
NSF Postdoctoral Fellow
University of Notre Dame
Title:
Dislodged & Ionized: Gaseous Structures of the Magellanic Clouds
Abstract:
Galaxy evolution is governed by an intricate ballet of gaseous inflows and outflows and galaxy interactions. The nearby Magellanic Clouds provides an advantageous opportunity to study these processes in detail. In this talk, we will explore the gas flows associated with these galaxies through H-alpha emission- and UV absorption-line observations. Galaxy interactions have greatly disturbed the Magellanic Clouds and have tidally displaced massive amounts of gas from these galaxies. These interactions have also triggered intense star formation throughout their disks; we provide compelling evidence that this elevated star formation drives even more material from these galaxies in wide spread, feedback driven winds. Through these observations, we determine the properties of these gas flows and explore their fates. We find that over a billion solar masses of gas neutral and ionized gas surrounds these galaxies. Much of this dislodged gas is transferring between the Magellanic Clouds and the Milky Way, depleting and replenishing their star formation gas reservoir respectively.
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