Your browser doesn't support javascript.
loading
A radio pulsar phase from SGR J1935+2154 provides clues to the magnetar FRB mechanism.
Zhu, Weiwei; Xu, Heng; Zhou, Dejiang; Lin, Lin; Wang, Bojun; Wang, Pei; Zhang, Chunfeng; Niu, Jiarui; Chen, Yutong; Li, Chengkui; Meng, Lingqi; Lee, Kejia; Zhang, Bing; Feng, Yi; Ge, Mingyu; Gögüs, Ersin; Guan, Xing; Han, Jinlin; Jiang, Jinchen; Jiang, Peng; Kouveliotou, Chryssa; Li, Di; Miao, Chenchen; Miao, Xueli; Men, Yunpeng; Niu, Chenghui; Wang, Weiyang; Wang, Zhengli; Xu, Jiangwei; Xu, Renxin; Xue, Mengyao; Yang, Yuanpei; Yu, Wenfei; Yuan, Mao; Yue, Youling; Zhang, Shuangnan; Zhang, Yongkun.
Afiliação
  • Zhu W; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Xu H; Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China.
  • Zhou D; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Lin L; Department of Astronomy, Peking University, Beijing 100871, China.
  • Wang B; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China.
  • Wang P; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Zhang C; University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China.
  • Niu J; Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China.
  • Chen Y; Department of Astronomy, Beijing Normal University, Beijing 100875, China.
  • Li C; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Meng L; Department of Astronomy, Peking University, Beijing 100871, China.
  • Lee K; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Zhang B; Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, China.
  • Feng Y; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Ge M; Department of Astronomy, Peking University, Beijing 100871, China.
  • Gögüs E; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Guan X; University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China.
  • Han J; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Jiang J; University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China.
  • Jiang P; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China.
  • Kouveliotou C; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Li D; University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing 100049, China.
  • Miao C; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Miao X; Department of Astronomy, Peking University, Beijing 100871, China.
  • Men Y; Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, China.
  • Niu C; Nevada Center for Astrophysics, University of Nevada, Las Vegas, NV 89154, USA.
  • Wang W; Department of Physics and Astronomy, University of Nevada, Las Vegas, NV 89154, USA.
  • Wang Z; Zhejiang Lab, Hangzhou, Zhejiang 311121, China.
  • Xu J; Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China.
  • Xu R; Faculty of Engineering and Natural Sciences, Sabanci University, 34956 Istanbul, Turkey.
  • Xue M; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Yang Y; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Yu W; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Yuan M; Department of Astronomy, Peking University, Beijing 100871, China.
  • Yue Y; National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.
  • Zhang S; Department of Physics, The George Washington University, 725 21st St. NW, Washington, DC 20052, USA.
  • Zhang Y; Max-Planck Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany.
Sci Adv ; 9(30): eadf6198, 2023 Jul 28.
Article em En | MEDLINE | ID: mdl-37506211
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Sci Adv Ano de publicação: 2023 Tipo de documento: Article País de afiliação: China
Texto completo
Imprimir
XML
PubMed Links
Buscar no Google

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Sci Adv Ano de publicação: 2023 Tipo de documento: Article País de afiliação: China