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Swift/UVOT discovery of Swift J221951−484240: a UV luminous ambiguous nuclear transient

Oates, SR; Kuin, NPM; Nicholl, M; Marshall, F; Ridley, E; Boutsia, K; Breeveld, AA; ... Xu, D; + view all (2024) Swift/UVOT discovery of Swift J221951−484240: a UV luminous ambiguous nuclear transient. Monthly Notices of the Royal Astronomical Society , 530 (2) pp. 1688-1710. 10.1093/mnras/stae795. Green open access

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Abstract

We report the discovery of Swift J221951−484240 (hereafter: J221951), a luminous slow-evolving blue transient that was detected by the Neil Gehrels Swift Observatory Ultraviolet/Optical Telescope (Swift/UVOT) during the follow-up of gravitational wave alert S190930t, to which it is unrelated. Swift/UVOT photometry shows the UV spectral energy distribution of the transient to be well modelled by a slowly shrinking blackbody with an approximately constant temperature of T ∼ 2.5 × 104 K. At a redshift z = 0.5205, J221951 had a peak absolute magnitude of Mu,AB = −23 mag, peak bolometric luminosity Lmax = 1.1 × 1045 erg s−1 and a total radiated energy of E > 2.6 × 1052 erg. The archival Wide-field Infrared Survey Explorer IR photometry shows a slow rise prior to a peak near the discovery date. Spectroscopic UV observations display broad absorption lines in N V and O VI, pointing towards an outflow at coronal temperatures. The lack of emission in the higher H α lines, N I and other neutral lines is consistent with a viewing angle close to the plane of the accretion or debris disc. The origin of J221951 cannot be determined with certainty but has properties consistent with a tidal disruption event and the turn-on of an active galactic nucleus.

Type: Article
Title: Swift/UVOT discovery of Swift J221951−484240: a UV luminous ambiguous nuclear transient
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/stae795
Publisher version: http://dx.doi.org/10.1093/mnras/stae795
Language: English
Additional information: This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third-party material in this article are included in the Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/
Keywords: Black hole physics, gravitational waves, galaxies: nuclei, ultraviolet: general, transients: tidal disruption events
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10192060
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