A 143 millisecond radio pulsar in the supernova remnant S147

被引:38
作者
Anderson, SB
Cadwell, BJ
Jacoby, BA
Wolszczan, A
Foster, RS
Kramer, M
机构
[1] PENN STATE UNIV,DEPT ASTRON & ASTROPHYS,UNIVERSITY PK,PA 16802
[2] USN,RES LAB,REMOTE SENSING DIV,WASHINGTON,DC 20375
[3] MAX PLANCK INST RADIOASTRON,D-53121 BONN,GERMANY
基金
美国国家科学基金会;
关键词
pulsars; individual (PSR J0538+2817); supernova remnants;
D O I
10.1086/310218
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of a 143 ms pulsar, PSR J0538+2817, in the supernova remnant S147 (0180.0-1.7). The pulsar is located 40' west of the center of S147, well within its evolved, roughly circular radio structure. An upper limit to the pulsar's age of 6x10(5) yr is consistent with the age of the remnant, estimated to be similar to(8 x 10(4))-(2 x 10(5)) yr. A dispersion measure-derived distance to PSR J0538+2817 is similar to 1.8 kpc, in reasonable agreement with a 0.8-1.6 kpc distance estimate for S147. These data provide sufficient evidence to hypothesize that the two objects are physically related and form a new association between a radio pulsar and an old supernova remnant.
引用
收藏
页码:L55 / L58
页数:4
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