ORBITAL ELEMENTS OF PSR B1620-26

被引:12
作者
MICHEL, FC
机构
[1] Space Phys. and Astronomy Department, Rice University, Houston
关键词
BINARIES; CLOSE; PULSARS; INDIVIDUAL (PSR B1620-26);
D O I
10.1086/174565
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We show that the third body around the binary pulsar B1620-26 can have virtually any mass. We also show that observations over the next decade should largely solve for the orbital elements of the system (with the usual exception of the inclination).
引用
收藏
页码:239 / 241
页数:3
相关论文
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[2]  
Michel F. C., 1991, THEORY NEUTRON STAR
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THORSETT, SE ;
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