AT2019 avd: A tidal disruption event with a two-phase evolution
Jin-Hong Chen, Li-Ming Dou, Rong-Feng Shen

TL;DR
This paper analyzes the tidal disruption event AT2019avd, revealing a two-phase evolution involving stream circularization and delayed accretion, with implications for SMBH properties and disk precession.
Contribution
It introduces a two-phase model for TDE evolution, combining self-crossing and delayed accretion models, and interprets X-ray variability as disk precession due to SMBH spin.
Findings
AT2019avd shows a double-peaked light curve with ~400 and 600 days durations.
The event is consistent with partial disruption of a 0.9 M_sun star by a 7 million solar mass SMBH.
X-ray variability suggests disk precession caused by SMBH spin with a period of 10-25 days.
Abstract
Tidal disruption events (TDEs) can uncover the quiescent supermassive black holes (SMBHs) at the center of galaxies. After the disruption of a star by a SMBH, the highly elliptical orbit of the debris stream will be gradually circularized due to the self-crossing, and then the circularized debris will form an accretion disk. The recent TDE candidate AT 2019avd has double peaks in its optical light curve, and the X-ray emerges near the second peak. The durations of the peaks are ~400 and 600 days, respectively, and the separation between them is ~700 days. We fit its spectral energy distribution (SED) and analyze its light curves in the optical/UV, mid-infrared, and X-ray bands. We find that this source can be interpreted as a two-phase scenario in which the first phase is dominated by the stream circularization, and the second phase is the delayed accretion. We use the succession of the…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Gamma-ray bursts and supernovae · Galaxies: Formation, Evolution, Phenomena
