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Mergers of white dwarfs (WDs) may lead to a variety of transientastrophysical events, SNIa being one possible outcome. Lyutikov & Toonen (2017,2019) argued that mergers of WDs result, under various parameter regimes, inunusual central engine-powered supernova and a type of short Gamma Ray Burststhat show extended emission tails. Observations by Gvaramadze et al. (2019) ofthe central star and the nebula J005311 match to the details the model ofLyutikov & Toonen (2017, 2019) for the immediate product of a merger of a heavyONeMg WD with CO WD (age, luminosity, stellar size, hydrogen deficiency andchemical composition).

Transients following white dwarfs mergers