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On the central engine of the fastest-declining Type I supernova SN2019bkc

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(2019)cite arxiv:1907.13271Comment: 3 pages, 1 figure. Res. Notes AAS, 3, 112 (2019).

Abstract

An analytic model is presented for the fastest-declining Type I supernova SN2019bkc. The model of the central engine consists of the magnetic dipole radiation from a non-explosive remnant of a double white dwarf merger. We consider the viscous evolution of the rotating remnant, which may lead to the diminishing energy supply in an appropriate time scale for the light curve.

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