We discuss the possible association of an astrophysical neutrino (IC220405B) with the recently reported, extremely energetic tidal disruption event (TDE) candidate AT2021lwx (ZTF20abrbeie, aka ``Scary Barbie'') at redshift $z=0.995$. Although the TDE is about $2.6^\circ$ off the direction of the reconstructed neutrino event (outside the 90% confidence level localization region), the TDE candidate shares some important characteristics with so far reported neutrino-TDE associations: a strong infrared dust echo, high bolometric luminosity, a neutrino time delay with respect to the peak mass accretion rate of the order of hundred days, and a high observed X-ray luminosity. We interpret this new association using an isotropic emission model, where neutrinos are produced by the collision of accelerated protons with infrared photons. After accounting for the high redshift of AT2021lwx (by interpreting the data in the SMBH frame), we find that the expected neutrino fluences and neutrino time delays are qualitatively comparable to the other TDEs. Since data are only available up to 300 days post-peak in the SMBH frame, significant uncertainties exist in the dust echo interpretation, and therefore in the predicted number of neutrinos detected, $\mathcal N_ν\simeq3.0\times10^{-3}-0.012$. We recommend further follow-up on this object for an extended period and suggest refining the reconstruction of the neutrino arrival direction in this particular case.
A Torus Remnant Revealed by the Infrared Echo of Tidal Disruption Event AT 2019qiz: Implications for the Missing Energy and Quasiperiodic Eruption Formation
Spectroscopic monitoring of the candidate tidal disruption event in F01004-2237
本文介绍了超亮红外星系F01004-2237的光谱监测观测结果。这个星系被观察到其光谱发生了变化，通过比较2015年的光谱和2000年的光谱来检测。这些变化与光度增亮一致。在光谱中检测到的主要变化是增强的He II $λ$ 4686发射和He I $λ$ 3898、$λ$ 5876发射线的出现。对这些变化的有利解释是2010年发生的潮汐中断事件（TDE）。然而，随后的工作表明，这些变化是由另一个迄今未知的原因引起的，与活动星系核（AGN）吸积率的变化有关。我们的光谱监测观测表明，He线的演化与TDE中观察到的演化一致，而与AGN混响绘图研究中观察到的演化相反，重新讨论了将耀斑解释为TDE的讨论。
Infrared observations reveal the reprocessing envelope in the tidal disruption event AT 2019azh
University of Turku（图尔库大学）；Niels Bohr Institute, University of Copenhagen（哥本哈根大学尼尔斯·玻尔研究所）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；University of Hong Kong（香港大学）；European University Cyprus（塞浦路斯欧洲大学）；Aalto University（阿尔托大学）；European Southern Observatory（欧洲南方天文台）；Universidad de Tarapacá（塔拉帕卡大学）；Tel Aviv University（特拉维夫大学）；Astronomical Observatory, University o（大学天文台）
A neutrino flare candidate potentially associated with X-ray emission from tidal disruption event ATLAS17jrp
Purple Mountain Observatory, Chinese Academy of Sciences（中国科学院紫金山天文台）；University of Science and Technology of China（中国科学技术大学）；Deutsches Elektronen-Synchrotron DESY（德国电子同步加速器）
研究发现一个可能与 tidal disruption 事件 ATLAS17jrp 发射的 X 射线相关的中微子喷流候选者，通过质子-光子过程产生中微子。
Triple radio flares from tidal disruption events: jet-wind collisions and the discovery of a third radio flare from AT2020vwl
School of Natural Sciences, Institute for Advanced Study（普林斯顿高等研究院自然科学学院）；International Centre for Radio Astronomy Research – Curtin University（西澳大学国际射电天文研究中心）；Department of Astronomy/Steward Observatory（天文学系/斯图尔德天文台）
Discovery of the luminous X-ray ignition eRASSt J234402.9$-$352640; I. Tidal disruption event or a rapid increase in accretion in an active galactic nucleus?
Testing the Association of Supermassive Black Hole Infrared Flares and High-energy Neutrinos
MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology（麻省理工学院）；Department of Astronomy and Columbia Astrophysics Laboratory, Columbia University（哥伦比亚大学）；Center for Computational Astrophysics, Flatiron Institute（西蒙斯基金会平顿研究所计算天体物理中心）；Department of Physics, Norwegian University of Science and Technology（挪威科技大学）
A Potential Second Shutoff from AT2018fyk: An updated Orbital Ephemeris of the Surviving Star under the Repeating Partial Tidal Disruption Event Paradigm
本文报告了 AT2018fyk 在 2023 年 8 月开始的 X 射线和紫外流量骤降，证实了重复部分潮汐瓦解事件（rpTDE）模型预测的第二次发射关闭，将轨道周期精确约束为 1306±47 天，并验证了 X 射线与 UV/光学发射追踪 SMBH 回落率的假设。
Early Near-Infrared Excess and Rapid Disk-Corona Evolution in the Tidal Disruption Event 2024aepd
Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences（中国科学院国家天文台光学天文重点实验室）；School of Astronomy and Space Sciences, University of Chinese Academy of Sciences（中国科学院大学天文与空间科学学院）；Tuorla observatory, Department of Physics and Astronomy, University of Turku（图尔库大学物理与天文学系图奥拉天文台）；Cosmic Dawn Center (DAWN)（宇宙黎明中心）；Niels Bohr Institute, University of Copenhagen（哥本哈根大学尼尔斯·玻尔研究所）；South-Western Institute for Astronomy Research, Yunnan University（云南大学西南天文研究所）；Department of Astronomy, Xiamen University（厦门大学天文学系）；Department of Astronomy, The University of Texas at Austin（德克萨斯大学奥斯汀分校天文学系）；The School of Physics and Astronomy, Te（物理学与天文学院）
Rapid onset of a Comptonisation zone in the repeating tidal disruption event XMMSL2 J140446.9-251135
Telespazio UK for ESA（ESA英国泰莱斯帕齐奥）；Schmidt Sciences（施密特科学）；Space Telescope Science Institute（太空望远镜科学研究所）；Leiden Observatory, Leiden University（莱顿大学莱顿天文台）；University of Arizona（亚利桑那大学）；Max-Planck-Institut für extraterrestrische Physik（马普地外物理研究所）；University of Hertfordshire（赫特福德大学）；University of Oxford（牛津大学）；Centro de Astrobiología (CAB), CSIC-INTA（CSIC-INTA天体生物学中心）；ESA（欧洲空间局）；SERCO for ESA（ESA塞科服务）
ATLAS22kjn (AT 2022fpx): A Coronal Line Emitter with an Early Light Curve Bump and Mid-Infrared Dust Echo
University of Illinois（伊利诺伊大学）；Institute for Astronomy, University of Hawai‘i（夏威夷大学天文研究所）；School of Physics, University of Melbourne（墨尔本大学物理学院）；The Ohio State University（俄亥俄州立大学）；Texas Tech University（德克萨斯理工大学）；Peking University（北京大学）；National Astronomical Observatories, Chinese Academy of Science（中国科学院国家天文台）
