【作者】Lingqi Meng，Weiwei Zhu，Michael Kramer，Xueli Miao，Gregory Desvignes，Lijing Shao，Huanchen Hu，Paulo C. C. Freire，Yongkun Zhang，Mengyao Xue，Ziyao Fang，David J. Champion，Mao Yuan，Chenchen Miao，Jiarui Niu，Qiuyang Fu，Jumei Yao，Yanjun Guo，Chengmin Zhang
【作者单位】1National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, People's Republic of China;2School of Astronomy and Space Science, University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China;3Institute for Frontiers in Astronomy and Astrophysics, Beijing Normal University, Beijing 102206, People's Republic of China;4Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany;5Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, University of Manchester, M13 9PL Manchester, UK;6Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing 100871, People's Republic of China;7The Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, People's Republic of China;8National Space Science Center, Chinese Academy of Sciences, Beijing 100190, People's Republic of China;9Research Institute of Artificial Intelligence, Zhejiang Lab, Hangzhou, Zhejiang 311121, People's Republic of China;10Xinjiang Astronomical Observatory, Chinese Academy of Sciences, 150, Science 1-Street, Urumqi, Xinjiang 830011, People's Republic of China
【年份】2024
【卷号】Vol.966 No.1
【页码】46
【ISSN】0004-637X
【摘要】 We observe systematic profile changes in the visible pulsar of the compact double neutron star system PSR J1946+2052 using observations with the Five-hundred-meter Aperture Spherical radio Telescope . The interpulse of PSR J1946+2052 changed from a s...
