Extreme variability in an active galactic nucleus: Gaia16aax
Hewett, P. C.; Kostrzewa-Rutkowska, Z.; Wevers, T.; Wyrzykowski, Ł.; Kankare, E.; Pringle, J. E.; Fraser, M.; Mattila, S.; Jonker, P. G.; Onori, F.; Nixon, C. J.; Cannizzaro, G.; Harmanen, J.; Ford, K. E. S.; McKernan, B.
Netherlands, Ireland, United Kingdom, Finland, Poland, Italy, United States
Abstract
We present the results of a multiwavelength follow-up campaign for the luminous nuclear transient Gaia16aax, which was first identified in 2016 January. The transient is spatially consistent with the nucleus of an active galaxy at z = 0.25, hosting a black hole of mass ∼ 6× 10^8 M_⊙. The nucleus brightened by more than 1 mag in the Gaia G band over a time-scale of less than 1 yr, before fading back to its pre-outburst state over the following 3 yr. The optical spectra of the source show broad Balmer lines similar to the ones present in a pre-outburst spectrum. During the outburst, the H α and H β emission lines develop a secondary peak. We also report on the discovery of two transients with similar light-curve evolution and spectra: Gaia16aka and Gaia16ajq. We consider possible scenarios to explain the observed outbursts. We exclude that the transient event could be caused by a microlensing event, variable dust absorption or a tidal encounter between a neutron star and a stellar mass black hole in the accretion disc. We consider variability in the accretion flow in the inner part of the disc, or a tidal disruption event of a star ≥ 1 M_{⊙} by a rapidly spinning supermassive black hole as the most plausible scenarios. We note that the similarity between the light curves of the three Gaia transients may be a function of the Gaia alerts selection criteria.