MAGNETIC MODELS OF PULSARS AND ROTATING NEUTRON STARS

被引:20
作者
GINZBURG, VL
ZAITSEV, VV
机构
[1] P. N. Lebedev Physical Institute, Academy of Sciences
关键词
D O I
10.1038/222230a0
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
The authors describe how magnetic models of pulsars can account for the narrowness of the beam of radiation. © 1969 Nature Publishing Group.
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页码:230 / &
相关论文
共 16 条
[1]  
Bratman V. L., 1968, Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki, V55, P1415
[2]   SECOND PERIODIC PULSATION IN PULSARS [J].
DRAKE, FD ;
CRAFT, HD .
NATURE, 1968, 220 (5164) :231-&
[3]  
GINZBURG VL, 1964, DOKL AKAD NAUK SSSR+, V156, P43
[4]   MAGNETIC MODELS OF PULSARS [J].
GINZBURG, VL ;
ZHELEZNYAKOV, VV ;
ZIATSEV, VV .
NATURE, 1968, 220 (5165) :355-+
[5]  
GINZBURG VL, 1964, ZH EKSP TEOR FIZ, V47, P1031
[6]  
GINZBURG VL, 1965, SOV PHYS JETP, V20
[7]  
GINZBURG VL, IN PRESS
[8]   ROTATING NEUTRON STARS AS ORIGIN OF PULSATING RADIO SOURCES [J].
GOLD, T .
NATURE, 1968, 218 (5143) :731-&
[9]  
KAPLAN SA, 1969, USPEKHI FIZ NAUK, V97
[10]   POSSIBLE MODEL FOR A RAPIDLY PULSATING RADIO SOURCE [J].
OSTRIKER, J .
NATURE, 1968, 217 (5135) :1227-&