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Fayin Wang

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Detection of X-ray emission from a bright long-period radio transient - Nature

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By Ziteng Wang, Nanda Rea, DAVID KAPLAN, Emil Lenc, Zorawar Wadiasingh, Andrew Zic, Apurba Kumar Bera, Paz Beniamini, A. J. Cooper, Tracy Clarke, J. R. Dawson, Marcin Glowacki, Natasha Hurley-Walker, S. J. McSweeney, Emil J. Polisensky, Wendy Peters, George Abi Younes, Keith Bannister, Manisha Caleb, Clancy W. James, Mansi Kasliwal, Kaya Mori, Stella Ocker, Miguel Pérez-Torres, Hao Qiu, Kovi Rose, Ryan Shannon, Fayin Wang, Yuanming Wang, Zhenyin Zhao, Laura N. Driessen, Tara Murphy, Joscha N. Jahns-Schindler
| Nature Verified
Abstract Recently, a class of long-period radio transients (LPTs) has been discovered, exhibiting emission thousands of times longer than radio pulsars1,2,3,4,5. These findings, enabled by advances in wide-field radio surveys, challenge existing models of rotationally powered pulsars. Proposed models include highly magnetized neutron stars6, white-dwarf pulsars7 and white-dwarf binary systems with low-mass companions8.
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