Disk-to-corona State Transition and Extreme X-Ray Variability in the Tidal Disruption Event AT2019teq

Abstract We present a 5 yr X-ray spectral and timing analysis of the optically selected tidal disruption event (TDE) AT2019teq, which displays extreme variability, including order-of-magnitude changes in flux on minute-to-day timescales, and a rare late-time emergence of hard X-ray emission leading to the longest-lived corona in a known TDE. In one epoch, we detect submillihertz quasiperiodic oscillations with significance tested via Markov Chain Monte Carlo based red-noise simulations ( p ≤ 0.03). AT2019teq exhibits a clear spectral evolution from a soft (blackbody-dominated) state to a hard (power-law-dominated) state, with a late-time radio brightening that may be associated with the state transition. We identify similarities between AT2019teq’s evolution and X-ray binary soft-to-hard state transitions, albeit at higher luminosity and much faster timescales. We use the presence of both the disk-dominated and corona-dominated states to apply multiple mass estimators from X-ray spectral and variability properties. These techniques are mutually consistent within 2 σ and systematically yield a lower BH mass ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">BH</mml:mi> </mml:mrow> </mml:msub> <mml:mo>/</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>5.67</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.09</mml:mn> </mml:math> ) than inferred from host galaxy scaling ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">BH</mml:mi> </mml:mrow> </mml:msub> <mml:mo>/</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>6.14</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.19</mml:mn> </mml:math> ).

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Journal
The Astrophysical Journal
Published
2026-03-09
DOI
https://doi.org/10.3847/1538-4357/ae3006
Primary Topic
Astrophysical Phenomena and Observations
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article
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article

Disk-to-corona State Transition and Extreme X-Ray Variability in the Tidal Disruption Event AT2019teq

Joheen Chakraborty, Megan Masterson, Vera L. Berger, Kevin B. Burdge et al.
The Astrophysical Journal
Astrophysical Phenomena and Observations
article

Disk-to-corona State Transition and Extreme X-Ray Variability in the Tidal Disruption Event AT2019teq

Joheen Chakraborty, Megan Masterson, Vera L. Berger, Kevin B. Burdge, Erin Kara
article en

Abstract

Abstract We present a 5 yr X-ray spectral and timing analysis of the optically selected tidal disruption event (TDE) AT2019teq, which displays extreme variability, including order-of-magnitude changes in flux on minute-to-day timescales, and a rare late-time emergence of hard X-ray emission leading to the longest-lived corona in a known TDE. In one epoch, we detect submillihertz quasiperiodic oscillations with significance tested via Markov Chain Monte Carlo based red-noise simulations ( p ≤ 0.03). AT2019teq exhibits a clear spectral evolution from a soft (blackbody-dominated) state to a hard (power-law-dominated) state, with a late-time radio brightening that may be associated with the state transition. We identify similarities between AT2019teq’s evolution and X-ray binary soft-to-hard state transitions, albeit at higher luminosity and much faster timescales. We use the presence of both the disk-dominated and corona-dominated states to apply multiple mass estimators from X-ray spectral and variability properties. These techniques are mutually consistent within 2 σ and systematically yield a lower BH mass ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">BH</mml:mi> </mml:mrow> </mml:msub> <mml:mo>/</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>5.67</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.09</mml:mn> </mml:math> ) than inferred from host galaxy scaling ( <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:mi>log</mml:mi> <mml:mo stretchy="false">(</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi mathvariant="normal">BH</mml:mi> </mml:mrow> </mml:msub> <mml:mo>/</mml:mo> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mo>⊙</mml:mo> </mml:mrow> </mml:msub> <mml:mo stretchy="false">)</mml:mo> <mml:mo>=</mml:mo> <mml:mn>6.14</mml:mn> <mml:mo>±</mml:mo> <mml:mn>0.19</mml:mn> </mml:math> ).

The Astrophysical JournalVol. 999(2)
Massachusetts Institute of Technology (US)
Peace, Justice and strong institutions
Openalex Percentile: Top 90%
Astrophysical Phenomena and Observations
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