The Astrophysical Journal Supplement Series (Jan 2024)

X-Ray Hardening Preceding the Onset of SGR 1935+2154's Radio Pulsar Phase

  • Pei Wang,
  • Jian Li,
  • Long Ji,
  • Xian Hou,
  • Erbil Gügercinoğlu,
  • Di Li,
  • Diego F. Torres,
  • Yutong Chen,
  • Jiarui Niu,
  • Wei-Wei Zhu,
  • Bing Zhang,
  • En-Wei Liang,
  • Li Zhang,
  • Mingyu Ge,
  • Zigao Dai,
  • Lin Lin,
  • Jinlin Han,
  • Yi Feng,
  • Chenhui Niu,
  • Yongkun Zhang,
  • Dejiang Zhou,
  • Heng Xu,
  • Chunfeng Zhang,
  • Jinchen Jiang,
  • Chenchen Miao,
  • Mao Yuan,
  • Weiyang Wang,
  • Dengke Zhou,
  • Jianhua Fang,
  • Youling Yue,
  • Yunsheng Wu,
  • Yabiao Wang,
  • Chengjie Wang,
  • Zhenye Gan,
  • Yuxi Li,
  • Zhongyi Sun,
  • Mingmin Chi,
  • Junshuo Zhang,
  • Jinhuang Cao,
  • Wanjin Lu,
  • Yidan Wang

DOI
https://doi.org/10.3847/1538-4365/ad7c3f
Journal volume & issue
Vol. 275, no. 2
p. 39

Abstract

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Magnetars are neutron stars with extremely strong magnetic fields, frequently powering high-energy activity in X-rays. Pulsed radio emission following some X-ray outbursts has been detected, albeit its physical origin is unclear. It has long been speculated that the origin of magnetars’ radio signals is different from those from canonical pulsars, although convincing evidence is still lacking. Five months after magnetar SGR 1935+2154's X-ray outburst and its associated fast radio burst 20200428, a radio pulsar phase was discovered. Here we report the discovery of X-ray spectral hardening associated with the emergence of periodic radio pulsations from SGR 1935+2154 and a detailed analysis of the properties of the radio pulses. The observations suggest that radio emission originates from the outer magnetosphere of the magnetar, and the surface heating due to the bombardment of inward-going particles from the radio emission region is responsible for the observed X-ray spectral hardening.

Keywords