Speaker
Prof.
Weiwei Zhu
(National Astronomical Observatories, Chinese Academy of Sciences)
Description
Pulsars and Fast Radio Bursts (FRB) are radio astronomy's most energetic and "fast" phenomena. They are both possibly from "neutron stars". In this talk, I will introduce some of my group and collaborators' pulsars and FRB research using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), from pulsar spin-kick geometry, emission geometry, relativistic spin precession in double neutron stars, to the emission geometry of FRB bursts in the magnetar SGR J1935+2154.
Primary author
Prof.
Weiwei Zhu
(National Astronomical Observatories, Chinese Academy of Sciences)
