A1 Journal article – refereed

Accretion disc cooling and narrow absorption lines in the tidal disruption event AT2019dsg




List of Authors: Cannizzaro G, Wevers T, Jonker PG, Perez-Torres MA, Moldon J, Mata-Sanchez D, Leloudas G, Pasham DR, Mattila S, Arcavi I, French KD, Onori F, Inserra C, Nicholl M, Gromadzki M, Chen TW, Muller-Bravo TE, Short P, Anderson JP, Young DR, Gendreau KC, Arzoumanian Z, Lowenstein M, Remillard R, Roy R, Hiramatsu D

Publisher: OXFORD UNIV PRESS

Publication year: 2021

Journal: Monthly Notices of the Royal Astronomical Society

Journal name in source: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Journal acronym: MON NOT R ASTRON SOC

Volume number: 504

Issue number: 1

Number of pages: 24

ISSN: 0035-8711

DOI: http://dx.doi.org/10.1093/mnras/stab851


Abstract
We present the results of a large multiwavelength follow-up campaign of the tidal disruption event (TDE) AT2019dsg, focusing on low to high resolution optical spectroscopy, X-ray, and radio observations. The galaxy hosts a super massive black hole of mass and careful analysis finds no evidence for the presence of an active galactic nucleus, instead the TDE host galaxy shows narrow optical emission lines that likely arise from star formation activity. The transient is luminous in the X-rays, radio, UV, and optical. The X-ray emission becomes undetected after similar to 100 d, and the radio luminosity density starts to decay at frequencies above 5.4 GHz by similar to 160 d. Optical emission line signatures of the TDE are present up to similar to 200 d after the light-curve peak. The medium to high resolution spectra show traces of absorption lines that we propose originate in the self-gravitating debris streams. At late times, after similar to 200 d, narrow Fe lines appear in the spectra. The TDE was previously classified as N-strong, but after careful subtraction of the host galaxy's stellar contribution, we find no evidence for these N lines in the TDE spectrum, even though O Bowen lines are detected. The observed properties of the X-ray emission are fully consistent with the detection of the inner regions of a cooling accretion disc. The optical and radio properties are consistent with this central engine seen at a low inclination (i.e. seen from the poles).

Downloadable publication

This is an electronic reprint of the original article.
This reprint may differ from the original in pagination and typographic detail. Please cite the original version.




Last updated on 2021-11-08 at 10:14