Seismological Studies of Pulsating DA White Dwarfs Observed with the Kepler Space Telescope and K2 Campaigns 1-8

Weston Hall, Barbara G. Castanheira, Agnès Bischoff-Kim

All single stars that are born with masses up to 8.5 - 10 $M_{\odot }$ will end their lives as a white dwarf (WD) star. In this evolutionary stage, WDs enter the cooling sequence, whe…