Radio Afterglows from Tidal Disruption Events: An Unbiased Sample from ASKAP RACS

被引:2
|
作者
Anumarlapudi, Akash [1 ]
Dobie, Dougal [2 ,3 ,4 ]
Kaplan, David L. [1 ]
Murphy, Tara [3 ,4 ]
Horesh, Assaf [5 ]
Lenc, Emil [6 ]
Driessen, Laura [4 ]
Duchesne, Stefan W. [7 ]
Dykaar, Hannah [8 ,9 ]
Gaensler, B. M. [8 ,9 ,10 ]
Galvin, Timothy J. [7 ,11 ]
Grundy, Joe [7 ,11 ]
Heald, George [7 ]
Hotan, Aidan W. [7 ]
Huynh, Minh [7 ]
Leung, James K. [5 ,8 ]
McConnell, David [6 ]
Moss, Vanessa A. [4 ,6 ]
Pritchard, Joshua [3 ,4 ,6 ]
Raja, Wasim [6 ]
Rose, Kovi [4 ,6 ]
Sivakoff, Gregory [12 ]
Wang, Yuanming [2 ,3 ]
Wang, Ziteng [11 ]
Wieringa, Mark H. [6 ]
Whiting, Matthew T. [6 ]
机构
[1] Univ Wisconsin Milwaukee, Dept Phys, POB 413, Milwaukee, WI 53201 USA
[2] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[3] ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
[4] Univ Sydney, Sydney Inst Astron, Sch Phys, Camperdown, NSW 2006, Australia
[5] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel
[6] CSIRO, Space & Astron, POB 76, Epping, NSW 1710, Australia
[7] CSIRO, Space & Astron, POB 1130, Bentley, WA 6102, Australia
[8] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[9] Univ Toronto, David A Dunlap Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada
[10] Univ Calif Santa Cruz, Dept Astron & Astrophys, 1156 High St, Santa Cruz, CA 95064 USA
[11] Curtin Univ, Int Ctr Radio Astron Res, 1 Turner Ave, Bentley, WA 6102, Australia
[12] Univ Alberta, Dept Phys, CCIS 4-181, Edmonton, AB T6G 2E1, Canada
来源
ASTROPHYSICAL JOURNAL | 2024年 / 974卷 / 02期
基金
澳大利亚研究理事会; 加拿大自然科学与工程研究理事会; 以色列科学基金会;
关键词
RELATIVISTIC OUTFLOW; EARLY EVOLUTION; DISCOVERY; NEARBY; STAR; VARIABILITY; POPULATION; FLARE; RATES; TDE;
D O I
10.3847/1538-4357/ad64d3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Late-time (similar to 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 22-11+15% 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 similar to 3 yr) of the survey. Finally, we project that the ongoing higher-cadence (similar to 2 months) ASKAP Variable and Slow Transients survey can detect similar to 20 TDEs in its operational span (4 yr), given the current rate from optical surveys.
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页数:15
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