INITIAL SPIN AND MAGNETIC-FIELD OF THE FAST PULSAR 4C21.53

被引：19

作者：

BRECHER, K ^{[1
]}

CHANMUGAM, G ^{[1
]}

机构：

[1] LOUISIANA STATE UNIV,DEPT PHYS & ASTRON,BATON ROUGE,LA 70803

来源：

NATURE | 1983年 / 302卷 / 5904期

关键词：

D O I：

10.1038/302124a0

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：124 / 125

页数：2

共 19 条

[1] A NEW CLASS OF RADIO PULSARS [J].

ALPAR, MA ;

CHENG, AF ;

RUDERMAN, MA ;

SHAHAM, J .

NATURE, 1982, 300 (5894) :728-730

[2] THE MAGNETIC-FIELDS OF WHITE-DWARFS [J].

ANGEL, JRP ;

BORRA, EF ;

LANDSTREET, JD .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1981, 45 (03) :457-474

[3]

ARONS J, NATURE

[4]

BACKER D, ANN NY ACAD SCI

[5] A MILLISECOND PULSAR [J].

BACKER, DC ;

KULKARNI, SR ;

HEILES, C ;

DAVIS, MM ;

GOSS, WM .

NATURE, 1982, 300 (5893) :615-618

[6] IMPROVED PARAMETERS FOR 67 PULSARS FROM TIMING OBSERVATIONS [J].

BACKUS, PR ;

TAYLOR, JH ;

DAMASHEK, M .

ASTROPHYSICAL JOURNAL, 1982, 255 (01) :L63-L67

[7] WHY DO COLLAPSED STARS ROTATE SO SLOWLY [J].

BRECHER, K ;

CHANMUGAM, G .

ASTROPHYSICAL JOURNAL, 1978, 221 (03) :969-972

[8] ADIABATIC STABILITY OF TOROIDAL MAGNETIC-FIELDS IN DIFFERENTIALLY ROTATING STARS [J].

CHANMUGAM, G .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1979, 187 (03) :769-776

[9] STABILITY OF FORCE-FREE MAGNETIC-FIELDS IN DEGENERATE STARS [J].

CHANMUGAM, G .

ASTROPHYSICAL JOURNAL, 1978, 221 (03) :965-968

[10] EVOLUTION OF PULSAR MAGNETIC-FIELDS [J].

FLOWERS, E ;

RUDERMAN, MA .

ASTROPHYSICAL JOURNAL, 1977, 215 (01) :302-310

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