ON THE ORIGIN OF THE 6.1-MS PULSAR

被引：80

作者：

JOSS, PC ^{[1
]}

RAPPAPORT, SA ^{[1
]}

机构：

[1] MIT,CTR THEORET PHYS,CAMBRIDGE,MA 02139

来源：

NATURE | 1983年 / 304卷 / 5925期

关键词：

D O I：

10.1038/304419a0

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：419 / 421

页数：3

共 19 条

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[2] A MILLISECOND PULSAR [J].

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[3]

BACKER DC, 1982, IAU3743 CIRC

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BUCCHERI, R ;

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NATURE, 1983, 304 (5925) :417-419

[5]

BORIAKOFF V, 1983, IAU3806 CIRC

[6] DO GALACTIC BULGE X-RAY SOURCES EVOLVE INTO MILLISECOND PULSARS [J].

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VERBUNT, F ;

WADE, RA .

NATURE, 1983, 301 (5897) :222-223

[7] OBSERVATIONAL CONSTRAINTS ON MASSES OF NEUTRON STARS [J].

JOSS, PC ;

RAPPAPORT, SA .

NATURE, 1976, 264 (5583) :219-222

[8] ACCRETING NEUTRON STARS IN HIGHLY COMPACT BINARY-SYSTEMS AND NATURE OF 3U 1626-67 [J].

JOSS, PC ;

AVNI, Y ;

RAPPAPORT, S .

ASTROPHYSICAL JOURNAL, 1978, 221 (02) :645-651

[9]

Landau L., 1962, CLASSICAL THEORY FIE

[10] TIDAL CIRCULARIZATION OF BINARY X-RAY SOURCES HERCULES X-1 AND CENTAURUS X-3 [J].

LECAR, M ;

WHEELER, JC ;

MCKEE, CF .

ASTROPHYSICAL JOURNAL, 1976, 205 (02) :556-562

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