Deep Searches for Radio Pulsations and Bursts from Four Magnetar and a Magnetar-like Pulsar with FAST

被引:0
|
作者
Bai, Juntao [1 ,2 ]
Wang, Na [1 ,3 ,4 ]
Dai, Shi [5 ,6 ]
Wang, Shuangqiang [1 ,3 ,4 ]
Yuan, Jianping [1 ,3 ,4 ]
Yan, Wenming [1 ,3 ,4 ]
Shang, Lunhua [7 ,8 ]
Xu, Xin [7 ,8 ]
Dang, Shijun [7 ,8 ]
Zhang, Zhen [1 ]
机构
[1] Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Xinjiang, Peoples R China
[2] Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
[3] Chinese Acad Sci, Key Lab Radio Astron, Urumqi 830011, Xinjiang, Peoples R China
[4] Xinjiang Key Lab Radio Astrophys, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China
[5] CSIRO Space & Astron, POB 76, Epping, NSW 1710, Australia
[6] Western Sydney Univ, Locked Bag 1797, Penrith, NSW 2751, Australia
[7] Guizhou Normal Univ, Sch Phys & Elect Sci, Guiyang 550001, Peoples R China
[8] Guizhou Normal Univ, Guizhou Prov Key Lab Radio Astron & Data Proc, Guiyang 550001, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2025年 / 979卷 / 02期
基金
中国国家自然科学基金;
关键词
FUNDAMENTAL PLANE; YOUNG PULSAR; EMISSION; OUTBURST; TELESCOPE; EVOLUTION; DISCOVERY;
D O I
10.3847/1538-4357/ada3c4
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on radio observations of four magnetars SGR 0501+4516, Swift 1834.9-0846, 1E 1841-045, SGR 1900+14, and a magnetar-like pulsar PSR J1846-0258 with the Five-hundred-meter Aperture Spherical radio Telescope at 1250 MHz. Notably, PSR J1846-0258 was observed 1 month after its 2020 X-ray outburst. The data from these observations were searched for periodic emissions and single pulses. No radio emission was detected for any of our targets. After accounting for the effect of red noise, the nondetections yield stringent upper limits on the radio flux density, with S1250 <= 16.9 mu Jy for the four magnetars and the magnetar-like pulsar, along with constraints on single-pulse flux densities. Our deep radio observations suggest that these magnetars and the magnetar-like pulsar are indeed radio-quiet sources or unfavorably beamed. The resulting flux upper limits, along with previous findings, are discussed, highlighting the significance of further radio observations of radio-quiet magnetars and the high-B magnetar-like pulsar.
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页数:5
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