PULSAR GEOMETRIES .3. HOLLOW-CONE MODEL

被引：26

作者：

OSTER, L

SIEBER, W

机构：

[1] UNIV COLORADO,JOINT INST LAB ASTROPHYS,DEPT PHYS & ASTROPHYS,BOULDER,CO 80309

[2] NBS,BOULDER,CO

[3] MAX PLANCK INST RADIOASTRON,BONN,FED REP GER

来源：

ASTROPHYSICAL JOURNAL | 1976年 / 210卷 / 01期

关键词：

D O I：

10.1086/154820

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：220 / 229

页数：10

共 17 条

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[2]

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[3]

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[4]

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TAYLOR, JH ;

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[6] POSSIBLE MECHANISM FOR PULSAR RADIO EMISSION [J].

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NATURE, 1970, 225 (5233) :612-+

[7] PULSAR GEOMETRIES .2. DECOMPOSITION OF RADIATION-PATTERN [J].

OSTER, L ;

SIEBER, W .

ASTROPHYSICAL JOURNAL, 1976, 203 (01) :233-244

[8] PULSAR GEOMETRIES - BASIC MODEL [J].

OSTER, L .

ASTROPHYSICAL JOURNAL, 1975, 196 (02) :571-577

[9] DRIFTING SUBPULSE PHENOMENON N PSR 0809 + 74 [J].

PAGE, CG .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 163 (01) :29-40

[10]

RADHAKRISHNAN V, 1969, ASTROPHYS LETT, V3, P225

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