Observational Constraints on the Origin of the Galactic center S-stars

Friday, January 24, 2020 - 12:15pm to 1:00pm
Devin Chu (UCLA)

The formation mechanism of the young S-stars located within an arcsecond of the supermassive black hole remains a mystery. Proposed formation scenarios for these S-stars include the tidal disruption of a binary system and migration from the clockwise disk of young stars.

TBD

Friday, February 7, 2020 - 12:15pm to 1:00pm
Katy Rodriguez Wimberly (UC Irvine)

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