Simulations of helium white dwarfs hit by supernova ejecta yield a tight relation between fractional mass loss and the ratio of ejecta ram pressure to donor pressure, matching several hypervelocity stars.
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Mass Loss and Subsequent Thermal Evolution of Surviving Helium White Dwarfs Shocked by Thermonuclear Supernovae
Simulations of helium white dwarfs hit by supernova ejecta yield a tight relation between fractional mass loss and the ratio of ejecta ram pressure to donor pressure, matching several hypervelocity stars.