Multiple tidal disruption flares in the active galaxy IC 3599
Abstract
Tidal disruption events occur when a star passes too close to a massive black hole and it is totally ripped apart by tidal forces. It may also happen that the star is not close enough to the black hole to be totally disrupted and a less dramatic event might happen. If the stellar orbit is bound and highly eccentric, just like some stars in the centre of our own Galaxy, repeated flares should occur. When the star approaches the black hole tidal radius at periastron, matter might be stripped resulting in lower intensity outbursts recurring once every orbital period. We report on Swift observations of a recent bright flare from the galaxy IC 3599 hosting a middle-weight black hole, where a possible tidal disruption event was observed in the early 1990s. By light curve modelling and spectral fitting we can consistently account for the events as the non-disruptive tidal stripping of a star into a highly eccentric orbit. The recurrence time is 9.5 yr. IC 3599 is also known to host a low-luminosity active galactic nucleus. Tidal stripping from this star over several orbital passages might be able to spoon-feed also this activity.
Cite
@article{arxiv.1502.07184,
title = {Multiple tidal disruption flares in the active galaxy IC 3599},
author = {S. Campana and D. Mainetti and M. Colpi and G. Lodato and P. D'Avanzo and P. A. Evans and A. Moretti},
journal= {arXiv preprint arXiv:1502.07184},
year = {2015}
}
Comments
Accepted for publication to Astronomy & Astrophysics