IGR J12580+0134: The First Tidal Disruption Event with an Off-beam Relativistic Jet
Abstract
Supermassive black holes (SMBHs) can capture and tidally disrupt stars or substellar objects orbiting nearby. The detections of Sw J1644+57-like events suggest that at least some TDEs can launch a relativistic jet beaming toward Earth. A natural expectation would be the existence of TDEs with a relativistic jet beaming away from Earth. The nearby TDE candidate IGR J12580+0134 provides new insights into the jet phenomenon. Combining several constraints, we find that the event invokes a 8-40 Jupiter mass object tidally disrupted by a 3× {10}5-1.8× {10}7{M}⊙ SMBH. Recently, a bright radio transient was discovered by Irwin et al. in association with IGR J12580+0134. We perform detailed modeling of the event based on a numerical jet model previously developed for the radio emission of Sw J1644+57. We find that the radio data of IGR J12580+0134 can be interpreted within an external forward shock model in the Newtonian regime. Using Sw J1644+57 as a template and properly correcting for its luminosity, we argue that the observed X-ray flux in early times is too faint to allow an on-beam relativistic jet unless the Lorentz factor is very small. Rather, the X-ray emission is likely from the disk or corona near the black hole. From various constraints, we find that the data are consistent with an off-beam relativistic jet with a viewing angle of {θ }{{obs}}≳ {30}{{o}}, and an initial Lorentz factor of {{{Γ }}}j≳ a few. This scenario can readily be tested in the upcoming very long baseline interferometry observations.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 2016
- DOI:
- 10.3847/0004-637X/816/1/20
- arXiv:
- arXiv:1511.01206
- Bibcode:
- 2016ApJ...816...20L
- Keywords:
-
- black hole physics;
- galaxies: individual: NGC 4845;
- galaxies: jets;
- X-rays: individual: IGR J12580+0134;
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 11 pages, 8 figures. Accepted for publication in ApJ