摘要
It is conjectured that coherent re-emission of cyclotron resonance absorption could result in pulsar giant pulses.This conjecture seems reasonable as it can naturally explain the distribution of pulsars with giant pulses on the P-P diagram.
作者
卢吉光
王维扬
彭勃
徐仁新
Ji-Guang Lu;Wei-Yang Wang;Bo Peng;Ren-Xin Xu(CAS Key Laboratory of FAST,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;Guizhou Radio Astronomy Observatory,Chinese Academy of Sciences,Guiyang 550025,China;Key Laboratory for Computational Astrophysics,National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China;University of Chinese Academy of Sciences,Beijing 100049,China;Department of Astronomy,Peking University,Beijing 100871,China;Kavli Institute for Astronomy and Astrophysics,Peking University,Beijing 100871,China)
基金
supported by the National Key R&D Program of China(Grant No.2018YFA0404703)
the National Natural Science Foundation of China(Grant Nos.11673002,12003047 and U1531243)
the Open Project Program of the Key Laboratory of FAST,NAOC,Chinese Academy of Sciences。
