Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4−055108

@article{Lin2020MultiwavelengthFO,
  title={Multiwavelength Follow-up of the Hyperluminous Intermediate-mass Black Hole Candidate 3XMM J215022.4−055108},
  author={Dacheng Lin and Jay Strader and Aaron J. Romanowsky and Jimmy A. Irwin and Olivier Godet and Didier Barret and Natalie Webb and Jeroen Homan and Ronald A. Remillard},
  journal={The Astrophysical Journal},
  year={2020}
}
We recently discovered the X-ray/optical outbursting source 3XMM J215022.4-055108. It was best explained as the tidal disruption of a star by an intermediate-mass black hole of mass of a few tens of thousand solar masses in a massive star cluster at the outskirts of a large barred lenticular galaxy at D_L=247 Mpc. However, we could not completely rule out a Galactic cooling neutron star as an alternative explanation for the source. In order to further pin down the nature of the source, we have… Expand

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