“脉冲星观测与理论研究”一般性科技报告  

Science Report of the Observations and Theory of Pulsar

作　　者：徐仁新[1] 

机构地区：[1]北京大学

出　　处：《科技创新导报》2016年第20期178-178,共1页Science and Technology Innovation Herald

摘　　要：在973项目(No.2012CB821800)支持下集中于射电脉冲星的若干理论与观测方面的研究。在利用新疆天文台25 m望远镜进行脉冲星常规观测的同时,课题组成员与云南天文台射电天文同行一起,建立了40 m望远镜脉冲星观测系统并进行初步观测、积累数据;成功运行了脉冲星搜寻软件,并用它处理了Parkes部分巡天数据,找到了部分脉冲星;继续研究脉冲星的磁层动力学过程与辐射机制、毫秒脉冲星与磁场的演化以及脉冲星内部的结构和致密物质状态的性质等,以便未来观测检验。The research of radio pulsars, from either theoretical or observational points of view, is focused under the financial support of the 973 project（No.2012CB821800）. Besides conventional radio pulsar monitoring using XJAO 25 m telescope, we are constructing a pulsar observation system of YNAO 40 m telescope. By running the pulsar searching code, we find a few pulsars from the Parkes survey data. The studies of pulsar magnetosphere and millisecond pulsar evolution, as well as pulsar inner structure are continued in order to have observational test by future advanced facilities.

关 键 词：脉冲星 中子星 夸克星 射电天文 致密物质 

分 类 号：P145.6[天文地球—天体物理]