White Dwarfs can go nova by accreting hydrogen from a neighbouring star; the gas is compressed by the extreme gravity of the white dwarf causing a thermonuclear runaway explosion on the surface (temperatures up to 20 million k). During a nova explosion, the energy released can equal what the sun emits over 10,000 years. The mass ejected only makes up about 1/10,000th of the white dwarfs mass, which means the star stays intact and can return to its prenova state. The process can be repeated every few thousand years.