AT 2023clx:在附近的恒星形成星系NGC 3799中发现的最微弱和最近的光学潮汐破坏事件

Jiazheng Zhu, N. Jiang, Ting-gui Wang, Shifeng Huang, Zheyu Lin, Yibo Wang, Jianguo Wang
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摘要

我们报告在附近的恒星形成星系NGC 3799中发现了一个微弱的光学潮汐破坏事件(TDE)。TDE的识别是基于它在星系核的位置,一个随t - 5/3衰减的光曲线,一个几乎恒定的黑体温度为~ 12,000 K的蓝色连续体,宽(≈15,000 km s - 1)的巴尔默线,以及He ii 4686 Å的特征发射。at2023clx的光曲线在g波段达到绝对星等为- 17.16等的峰值,黑体的最大热光度为4.56 × 1042 erg s - 1,是迄今为止发现的最微弱的TDE。它的红移为0.01107,对应的光度距离为47.8 Mpc,这也是迄今为止发现的最接近我们所知的光学TDE。此外,我们对AT 2023clx的Swift/XRT观测结果的分析在0.3-10 keV范围内得到了9.53 × 1039 erg s−1的非常严格的3σ上限。at2023clx和极少数微弱的tde,如at2020wey,证明在更高的红移上可能有大量的微弱tde尚未被发现,这与光度函数(LFs)的预测是一致的。即将进行的更深入的光学时域巡天,如传统时空巡天和宽视场巡天望远镜,将在更低的光度下发现更多的tde,从而更精确地约束LF的低端。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
AT 2023clx: The Faintest and Closest Optical Tidal Disruption Event Discovered in Nearby Star-forming Galaxy NGC 3799
We report the discovery of a faint optical tidal disruption event (TDE) in the nearby star-forming galaxy NGC 3799. Identification of the TDE is based on its position at the galaxy nucleus, a light curve declining as t −5/3, a blue continuum with an almost constant blackbody temperature of ∼12,000 K, broad (≈15,000 km s−1) Balmer lines, and characteristic He ii 4686 Å emission. The light curve of AT 2023clx peaked at an absolute magnitude of −17.16 mag in the g band and a maximum blackbody bolometric luminosity of 4.56 × 1042 erg s−1, making it the faintest TDE discovered to date. With a redshift of 0.01107 and a corresponding luminosity distance of 47.8 Mpc, it is also the closest optical TDE ever discovered to the best of our knowledge. Furthermore, our analysis of Swift/XRT observations of AT 2023clx yields a very tight 3σ upper limit of 9.53 × 1039 erg s−1 in the range 0.3–10 keV. AT 2023clx, together with very few other faint TDEs such as AT 2020wey, prove that there are probably a large number of faint TDEs yet to be discovered at higher redshifts, which is consistent with the prediction of luminosity functions (LFs). The upcoming deeper optical time-domain surveys, such as the Legacy Survey of Space and Time and the Wide Field Survey Telescope, will discover more TDEs at even lower luminosities, allowing for a more precise constraint of the low end of the LF.
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