blue, red, and green computer-generated graphic.

Computer simulation of a burning front moving upward through a channel distorted by strong turbulence. This burning front is similar to that which incinerates a star in about a second during a thermonuclear supernova. The red surface is the forward side of the front and the blue is the back. Simulation by UA faculty member Dean Townsley.

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Colloquium Speaker: Jamie Tayar (University of Hawaii)

March 8 @ 2:00 pm
Virtual

Dr. Jamie Tayar will give a colloquium on Re-envisioning Stellar Physics in the Time Domain Era

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Colloquium Speaker: Matthew Shultz (University of Delaware)

March 10 @ 3:30 pm
Virtual

Dr. Matthew Shultz will give a colloquium on Magnetic Fields and Magnetospheres of Hot Stars

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Colloquium Speaker: Dom Walton (University of Cambridge)

March 17 @ 3:30 pm
Virtual

Dr. Dom Walton will give a colloquium on Putting a Spin on Black Holes in the NuSTAR Era

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Colloquium Speaker: Burcin Mutlu-Pakdil (University of Chicago)

March 24 @ 3:30 pm
Virtual

Dr. Burcin Mutlu-Pakdil will give a colloquium on The Smallest and Faintest Galaxies: Clues to the Nature of Dark Matter and Galaxy Formation

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