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Extensive observations from the Kepler spacecraft have recently revealed anew outburst phenomenon operating in cool pulsating DA (hydrogen atmosphere)white dwarfs (DAVs). With the introduction of two new outbursting DAVs from K2Fields 7 (EPIC 229228364) and 8 (EPIC 220453225) in these proceedings, wepresently know of six total members of this class of object. We present theobservational commonalities of the outbursting DAVs: (1) outbursts thatincrease the mean stellar flux by up to 15%, last many hours, and recurirregularly on timescales of days; (2) effective temperatures that locate themnear the cool edge of the DAV instability strip; and (3) rich pulsation spectrawith modes that are observed to wander in amplitude/frequency.

The First Six Outbursting Cool DA White Dwarf Pulsators