| Issue |
A&A
Volume 708, April 2026
|
|
|---|---|---|
| Article Number | L20 | |
| Number of page(s) | 7 | |
| Section | Letters to the Editor | |
| DOI | https://doi.org/10.1051/0004-6361/202558455 | |
| Published online | 24 April 2026 | |
Letter to the Editor
Similar ratios of the rise timescale to the decline timescale of optical light curves in common tidal disruption events
Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, GuangXi University, No. 100, Daxue Road, Nanning 530004, P.R. China
★ Corresponding author: This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
8
December
2025
Accepted:
29
March
2026
Abstract
The entirely similar physical process in tidal disruption events (TDEs) basically indicates that just one parameter might distinguish the variability properties of TDEs from that of other transient events that have different physical processes. We report such a parameter, the timescale ratio R2/1, rd of the rise timescale t1/2, r (from half maximum to maximum) to the decline timescale t1/2, d (from maximum to half maximum). We define this based on 34 optical TDEs with reported t1/2, r and t1/2, d. Among the 34 optical TDEs, AT2020wey is an outlier with R2/1, rd ∼ 2.7, which is 4.5 times higher than the mean value 0.6 of the other optical TDEs. However, when the similar but more flexible model functions are considered, the redetermined R2/1, rd is ∼0.9 in AT2020wey. This is very similar to the values of the other optical TDEs. Therefore, the parameter R1/2, rd ∼ 0.6 might be a potential classification parameter for optical TDEs. Furthermore, R1/2, rd were determined in the unique optical transients AT2019avd, PS1-10adi, SDSS J0946+3512, and J2334+1457. The second flare with R1/2, rd ∼ 11 in AT2019avd is expected to be very different from that of other optical TDEs, but PS1-10adi, SDSS J0946+3512, J2334+1457, and the first flare in AT2019avd are expected to be similar to the other optical TDEs. In the near future, the properties of R1/2, rd determined on a large sample of optical transients might provide further clues to support whether R1/2, rd might be a better classification parameter to distinguish TDEs from other transient events.
Key words: galaxies: active / galaxies: nuclei / quasars: supermassive black holes
© The Authors 2026
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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