A DETERMINATION OF THE WHITE-DWARF MASSES IN WIDE BINARY RADIO-PULSAR SYSTEMS

被引：56

作者：

SAVONIJE, GJ

机构：

来源：

NATURE | 1987年 / 325卷 / 6103期

关键词：

D O I：

10.1038/325416a0

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：416 / 418

页数：3

共 13 条

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[2]

DEKOOL M, 1986, ASTRON ASTROPHYS, V164, P73

[3] BINARY PULSAR WITH A VERY SMALL MASS FUNCTION [J].

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MAGUIRE, CM ;

RAWLEY, LA ;

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

JOSS, PC ;

RAPPAPORT, SA .

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

[5]

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[6] OPTICAL-IDENTIFICATION OF BINARY PULSARS - IMPLICATIONS FOR MAGNETIC-FIELD DECAY IN NEUTRON-STARS [J].

KULKARNI, SR .

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[7] EVOLUTIONARY HISTORY OF THE 6.1-MS PULSAR [J].

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NATURE, 1983, 304 (5925) :421-422

[8] EVOLUTIONARY PROCESSES IN CLOSE BINARY SYSTEMS [J].

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ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1971, 9 :183-+

[9] IS THE 6-MS BINARY PULSAR THE REMNANT OF A BRIGHT GALACTIX X-RAY SOURCE [J].

SAVONIJE, GJ .

NATURE, 1983, 304 (5925) :422-423

[10]

SAVONIJE GJ, 1985, INTERACTING BINARIES, P83

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