Search for Fast Radio Bursts and Radio Pulsars from Pulsing Ultraluminous X-Ray Sources

被引:0
作者
Bai, Juntao [1 ,2 ]
Wang, Na [1 ,3 ]
Luo, Rui [4 ]
Wang, Wei-Yang [2 ]
Dai, Shi [5 ,6 ]
Zhang, Songbo [7 ]
Zhao, Shiqian [4 ]
Wang, Shuangqiang [1 ,3 ,5 ]
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] Guangzhou Univ, Sch Phys & Mat Sci, Dept Astron, Guangzhou 510006, 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] Chinese Acad Sci, Purple Mt Observ, Nanjing 210023, Peoples R China
基金
中国国家自然科学基金;
关键词
COHERENT CURVATURE RADIATION; SYNCHROTRON MASER EMISSION; NEUTRON-STAR; BINARY; DISCOVERY; MAGNETAR; BUNCHES; ULX1;
D O I
10.3847/1538-4357/adc92e
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We conducted targeted fast radio burst (FRB) and pulsar searches on eight pulsing ultraluminous X-ray sources (PULXs) using the Five-hundred-meter Aperture Spherical radio Telescope (FAST) and the Parkes 64 m Radio Telescope (Murriyang) to investigate whether PULXs could be progenitors of FRBs. FAST carried out 12 observations of four PULXs, totaling 8 hr, while Parkes conducted 12 observations of the remaining four PULXs, totaling 11 hr. No significant signals were detected through single-pulse and periodic searches, covering a dispersion measure range of 0-5000 pc cm-3, placing stringent upper limits on the radio flux density from these sources. The results imply that accretion processes and dense stellar winds in PULXs likely suppress or attenuate potential coherent emission in the radio band. Additionally, the beaming factor and luminosity of FRBs associated with PULXs, as well as the highly relativistic and magnetized nature of their outflows, may limit detectability. Nondetection yielded from the observations covering the full orbital phases of PULXs can also constrain the theoretical models that link FRB emission to highly magnetized neutron stars in binary systems.
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页数:6
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