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arXiv 2410.09720astro-ph.HEastro-ph.GA
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IRAS F01004-2237中相隔十年的复发潮汐瓦解事件

Recurring tidal disruption events a decade apart in IRAS F01004-2237

Luming Sun, Ning Jiang, Liming Dou, Xinwen Shu, Jiazheng Zhu, Subo Dong, David Buckley, S. Bradley Cenko, Xiaohui Fan, Mariusz Gromadzki, Zhu Liu, Jianguo Wang,… 展开作者

Luming Sun, Ning Jiang, Liming Dou, Xinwen Shu, Jiazheng Zhu, Subo Dong, David Buckley, S. Bradley Cenko, Xiaohui Fan, Mariusz Gromadzki, Zhu Liu, Jianguo Wang, Tinggui Wang, Yibo Wang, Tao Wu, Lei Yang, Fabao Zhang, Wenjie Zhang, Xiaer Zhang

AI总结:

本研究在IRAS F01004-2237中发现了相隔约10.3年的第二次光学耀斑,通过多波段分析确认其为潮汐瓦解事件,并探讨了其作为重复部分TDE或独立TDE的可能性及未来观测预测。

摘要:

我们报告了在IRAS F01004-2237中发现的第二次光学耀斑,该耀斑发生于2021年9月,而此前已报告过该星系在2010年发生的首次耀斑,并在此呈现多波段数据的详细分析。耀斑位置与星系中心重合,精度为650 pc。耀斑在约50天内达到峰值,绝对星等约为-21,并在两年内衰减,大致遵循$L\propto t^{-5/3}$的规律。在后期,它保持约22,000 K的几乎恒定的黑体温度。其光学和紫外光谱显示出氢和氦的宽发射线,半高全宽为7,000--21,000 km s$^{-1}$,He II/H$α$比值为0.3--2.3。相对于紫外辐射,它表现出较弱的X射线发射,X射线耀斑持续不到2-3周,期间光谱较软,幂律指数为$Γ=4.4^{+1.4}_{-1.3}$。这些特征与潮汐瓦解事件(TDE)一致,排除了超新星或活动星系核耀斑的可能性。使用TDE模型,我们推断峰值紫外光度为$3.3\pm0.2\times10^{44}$ erg s$^{-1}$,能量预算为$4.5\pm0.2\times10^{51}$ erg。相隔$10.3\pm0.3$年的两次光学耀斑可被解释为重复的部分TDE、双TDE或两次独立的TDE。尽管尚无定论,但部分TDE解释预测在2033年左右会出现第三次耀斑,而独立TDE解释预测F01004-2237中的TDE发生率较高($\gtrsim10^{-2}$ yr$^{-1}$),两者均可通过未来观测进行检验。

英文摘要:

We report the discovery of a second optical flare that occurred in September 2021 in IRAS F01004-2237, where the first flare occurred in 2010 has been reported, and present a detailed analysis of multi-band data. The position of the flare coincides with the galaxy centre with a precision of 650 pc. The flare peaks in $\sim50$ days with an absolute magnitude of $\sim-21$ and fades in two years roughly following $L\propto t^{-5/3}$. It maintains a nearly constant blackbody temperature of $\sim$22,000 K in the late time. Its optical and UV spectra show hydrogen and helium broad emission lines with full width at half maxima of 7,000--21,000 km s$^{-1}$ and He II/H$α$ ratio of 0.3--2.3. It shows weak X-ray emission relative to UV emission, with X-ray flares lasting for $<2-3$ weeks, during which the spectrum is soft with a power-law index $Γ=4.4^{+1.4}_{-1.3}$. These characters are consistent with a tidal disruption event (TDE), ruling out the possibilities of a supernova or an active galactic nuclei flare. With a TDE model, we infer a peak UV luminosity of $3.3\pm0.2\times10^{44}$ erg s$^{-1}$ and an energy budget of $4.5\pm0.2\times10^{51}$ erg. The two optical flares separated by $10.3\pm0.3$ years can be interpreted as repeating partial TDEs, double TDEs, or two independent TDEs. Although no definitive conclusion can be drawn, the partial TDEs interpretation predicts a third flare around 2033, and the independent TDEs interpretation predicts a high TDE rate of $\gtrsim10^{-2}$ yr$^{-1}$ in F01004-2237, both of which can be tested by future observations.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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