PERIOD DERIVATIVE AND ORBITAL ECCENTRICITY OF BINARY PULSAR 1953+29

被引：31

作者：

RAWLEY, LA

TAYLOR, JH

DAVIS, MM

机构：

[1] PRINCETON UNIV,DEPT PHYS,PRINCETON,NJ 08544

[2] ARECIBO OBSERV,ARECIBO,PR 00613

来源：

NATURE | 1986年 / 319卷 / 6052期

关键词：

D O I：

10.1038/319383a0

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：

引用

页码：383 / 384

页数：2

共 18 条

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[4]

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[6]

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[7] ASSOCIATION OF THE 6-MS PULSAR PSR1953 WITH THE COS-B GAMMA-RAY SOURCE 2CG065 [J].

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[8]

CHANDLER JF, 1984, PEP740R PREPR

[9] ON THE ORIGIN OF THE 6.1-MS PULSAR [J].

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NATURE, 1983, 304 (5925) :419-421

[10]

LOREDO TJ, 1984, MILLISECOND PULSARS, P48

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