潮汐扰动事件的射电余辉:来自 ASKAP RACS 的无偏样本

Akash Anumarlapudi, Dougal Dobie, David L. Kaplan, Tara Murphy, Assaf Horesh, Emil Lenc, Laura Driessen, Stefan W. Duchesne, Hannah Dykaar, B. M. Gaensler, Timothy J. Galvin, Joe Grundy, George Heald, Aidan W. Hotan, Minh Huynh, James K. Leung, David McConnell, Vanessa A. Moss, Joshua Pritchard, Wasim Raja, Kovi Rose, Gregory Sivakoff, Yuanming Wang, Ziteng Wang, Mark H. Wieringa and Matthew T. Whiting
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摘要

对光学发现的潮汐扰动事件(TDEs)的晚期(∼a 年)射电跟踪越来越多地导致在射电波长上的探测,越来越多的证据表明这种晚期射电活动是亚相对论 TDEs 大类的共同特征。对其中一些射电波长 TDE 的详细研究也对现有的射电发射模型提出了挑战。利用澳大利亚平方千米阵列探路者(ASKAP)的全天空多历元数据,作为快速ASKAP连续巡天(RACS)的一部分,我们搜索了光学发现的TDEs样本的射电对应物。我们在五颗 TDEs 中探测到了 RACS 频率(742-1032 MHz)的晚期发射,报告了从 TDE AT 2019ahk 中独立发现的射电发射,并将一些事件的时间基线延长到了近 3000 天。总之,我们发现在光学发现的TDE中,至少有一部分在RACS巡天中具有可探测到的射电辐射,同时我们也注意到,由于巡天的周期有限(两个历元相隔∼3年),真正的比例可能会更高。最后,我们预计正在进行的更高频率(∼2 个月)的 ASKAP 变慢瞬变巡天在其工作时间跨度(4 年)内可以探测到 ∼20 个 TDEs,考虑到目前光学巡天的探测率。
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Radio Afterglows from Tidal Disruption Events: An Unbiased Sample from ASKAP RACS
Late-time (∼a year) radio follow-up of optically discovered tidal disruption events (TDEs) is increasingly resulting in detections at radio wavelengths, and there is growing evidence for this late-time radio activity to be common to the broad class of subrelativistic TDEs. Detailed studies of some of these TDEs at radio wavelengths are also challenging the existing models for radio emission. Using all-sky multiepoch data from the Australian Square Kilometre Array Pathfinder (ASKAP), taken as a part of the Rapid ASKAP Continuum Survey (RACS), we searched for radio counterparts to a sample of optically discovered TDEs. We detected late-time emission at RACS frequencies (742–1032 MHz) in five TDEs, reporting the independent discovery of radio emission from TDE AT 2019ahk and extending the time baseline out to almost 3000 days for some events. Overall, we find that at least of the population of optically discovered TDEs has detectable radio emission in the RACS survey, while also noting that the true fraction can be higher given the limited cadence (two epochs separated by ∼3 yr) of the survey. Finally, we project that the ongoing higher-cadence (∼2 months) ASKAP Variable and Slow Transients survey can detect ∼20 TDEs in its operational span (4 yr), given the current rate from optical surveys.
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