A PULSAR SUPERNOVA ASSOCIATION

被引：181

作者：

LARGE, MI

VAUGHAN, AE

MILLS, BY

机构：

[1] Cornell-Sydney University Astronomy Centre, School of Physics

来源：

NATURE | 1968年 / 220卷 / 5165期

关键词：

D O I：

10.1038/220340a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

A pulsar with a very short period (0.089 s) has been discovered at the position of a suspected supernova remnant, raising several interesting consequences. © 1968 Nature Publishing Group.

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页码：340 / &

相关论文

共 7 条

[1] ACCURATE POSITION OF A SECOND PULSED RADIO SOURCE
BAILEY, JA
MACKAY, CD
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[2] OBSERVATION OF A RAPIDLY PULSATING RADIO SOURCE
HEWISH, A
BELL, SJ
PILKINGT.JD
SCOTT, PF
COLLINS, RA
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[3] A CATALOGUE OF GALACTIC RADIO SOURCES
KESTEVEN, MJ
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[4] RADIO EMMISSION FROM SUPERNOVA REMNANT VELA-X
MILNE, DK
[J]. AUSTRALIAN JOURNAL OF PHYSICS, 1968, 21 (02): : 201 - &
[5] WHITE-DWARF AND NEUTRON-STAR INTERPRETATIONS OF PULSATING RADIO SOURCES
THORNE, KS
IPSER, JR
[J]. ASTROPHYSICAL JOURNAL, 1968, 152 (1P2) : L71 - &
[6] POSITIONS OF 4 PULSARS
TURTLE, AJ
VAUGHAN, AE
[J]. NATURE, 1968, 219 (5156) : 845 - &
[7] DISCOVERY OF 2 SOUTHERN PULSARS
TURTLE, AJ
VAUGHAN, AE
[J]. NATURE, 1968, 219 (5155) : 689 - &