This research investigates extreme binary star systems containing white dwarfs using a multi-wavelength astronomical approach. The study discovered new low-level mass transfer systems, provided evidence for theories of white dwarf magnetism, and identified mysterious radio sources as magnetic binary systems. These findings improve understanding of high-energy astrophysical processes and stellar evolution.

My talk explains how neutron stars—extremely dense remnants of stellar explosions—contain matter we cannot study on Earth. By analyzing gravitational waves from colliding neutron stars, the speaker models how their deformation (or “squishiness”) reveals their internal composition. This method may uncover entirely new forms of matter and transform fundamental physics.