Abstract

In March 2011 Swift detected an extremely luminous and long-lived outburst from the nucleus of an otherwise quiescent, low luminosity (LMC-like) galaxy. Named Swift J1644+57, its combination of high-energy luminosity (1048 ergs s−1 at peak), rapid X-ray variability (factors of >100 on timescales of 100 seconds) and luminous, rising radio emission suggested that we were witnessing the birth of a moderately relativistic jet (Γ ∼ 2 − 5), created when a star is tidally disrupted by the supermassive black hole in the centre of the galaxy. A second event, Swift J2058+0516, detected two months later, with broadly similar properties lends further weight to this interpretation. Taken together this suggests that a fraction of tidal disruption events do indeed create relativistic outflows, demonstrates their detectability, and also implies that low mass galaxies can host massive black holes. Here, I briefly outline the observational properties of these relativistic tidal flares observed last year, and their evolution over the first year since their discovery.

Highlights

  • On the 28th March 2011 the Swift satellite detected what appeared at first to be a very long duration gamma-ray burst (GRB 110328A), detected as an image trigger with a duration of over twenty minutes [1]

  • An analysis of archival images of the field revealed a quiescent counterpart with R ∼ 22 in the X-ray error box [3]

  • Combined with the luminous X-ray afterglow these properties appeared at first sight similar to those of the Supergiant Fast X-ray Transients – High mass X-ray binaries with our Galaxy [4]

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Summary

Introduction

On the 28th March 2011 the Swift satellite detected what appeared at first to be a very long duration gamma-ray burst (GRB 110328A), detected as an image trigger with a duration of over twenty minutes [1]. Our observations unveiled a faint, fading infrared counterpart [6], which would provide a precise position for the burst relative to this host galaxy [7]. The X-ray afterglow was seen to persist at a bright level (>10−10 ergs s−1 cm−2) for several days, and subsequently re-triggered the BAT on two further occasions (i.e. triggered it four times in total) [2].

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