Nov 29, 2018

Tom Maccarone, Texas Tech University

""Surveying the Galactic Bulge for Transients and Compact Binaries""

Understanding the evolution of binary stars is vital for almost all of the key problems in astrophysics today.  For example, gravitational wave sources and Type Ia supernovae are fundamentally binary processes.  From a theoretical point of view, binary stellar evolution is extremely complicated, with many poorly understood processes contributing.  To build up an understanding of binary evolution, it is thus necessary to build a set of observational constraints.  Here, I will present the results from several projects aimed at understanding the binary and transient populations of the Milky Way's Galactic Bulge.  Some key highlights will include new understanding of cataclysmic variables, accreting black holes and neutron stars, and the discovery of a low mass protostar that appears to have formed in isolation.
 

Event Details

Date:
Nov 29, 2018

Time:
3:30–5pm

Location:
4421 Stering Hall

Notes:
Coffee served at 3:30pm; talk starts at 3:45pm

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