ON THE YOUNG CRAB-LIKE SNRs AND THEIR STATISTICAL L_x-E RELATION  

作　　者：陈阳 曲钦岳 汪珍如 

机构地区：[1]Department of Astronomy, Nanjing University, Nanjing 210008, PRC

出　　处：《Chinese Science Bulletin》1992年第24期2062-2066,共5页

基　　金：Project supported by the National Natural Science Foundation of China

摘　　要：Crab-like supernova remnants (plerions) are a kind of SNR which has a central neutron star or pulsar. It is generally believed that the central pulsar drives the evolution of the plerion. A statistical relation between the soft X-ray (0.2—4 keV )luminosity L_x of the synchrotron nebula (including the pulsar)and the pulsar rotating energy loss rate

关 键 词：SUPERNOVA REMNANTS the CRAB NEBULA X-ray sources 

分 类 号：N[自然科学总论]