Faint rapid red transients from Neutron star -- CO white-dwarf mergers

Mergers of neutron stars (NS) and white dwarfs (WD) may give rise to observable explosive transient events. We use 3D hydrodynamical (SPH) simulations, as well as 2D hydrodynamical-thermonuclear simulations (using the FLASH AMR code) to model the disruption of CO-WDs by NSs, which produce faint transient events. We post-process the simulations using a large nuclear network and make use of the SuperNu radiation-transfer code to predict the observational signatures and detailed properties of these transients. We calculate the light-curves (LC) and spectra for five models of NS - CO-WD mergers. The small yields of Ni56 (few x 0.001Msun) results in faint, rapidly-evolving reddened transients (RRTs) with B (R) - peak magnitudes of ~ -12 (-13) to ~ -13 (-15), much shorter and fainter than both regular and faint/peculiar type-Ia SNe. We show that the spectra of RRTs share some similarities with rapidly - evolving transients such as SN2010x, though RRTs are significantly fainter, especially in the I/R bands, and show far stronger Si lines. We estimate that the upcoming Large Synoptic Survey Telescope could detect RRTs at a rate of ~ 10 - 70 yr^-1, through observations in the R/I bands.

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