Pulsar transient radio emission
Radiation processes in the closed field line regions of pulsar magnetospheres are discussed. It is argued that trapped particles form radiation belts in the closed field line regions in the majority of pulsars. It is proposed that transient radio emission, seen as rotating radio transients (RRATs), results from events that trigger precipitation of these trapped particles.
pulsars radiation mechanism-nonthermal particle acceleration
Qinghuan Luo Don Melrose
School of Physics, The University of Sydney, NSW 2006, Australia
国际会议
紧凑型物体的天体物理学国际会议(International Conference on Astrophysics of Compact Objects)
安徽黄山
英文
159-164
2007-07-01(万方平台首次上网日期,不代表论文的发表时间)