FREQUENCY-DEPENDENCE OF CHARACTERISTICS OF PULSARS PSR0031-07, 0320+39, 1133+16 AND 2016+28

被引：24

作者：

IZVEKOVA, VA ^{[1
]}

KUZMIN, AD ^{[1
]}

LYNE, AG ^{[1
]}

SHITOV, YP ^{[1
]}

SMITH, FG ^{[1
]}

机构：

[1] UNIV MANCHESTER,NUFFIELD RADIO ASTRON LABS,MACCLESFIELD SK11 9DL,CHESHIRE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1993年 / 261卷 / 04期

关键词：

PULSARS; INDIVIDUAL; PSR0031-07; PSR0320+39; PSR1133+16; PSR2016+28; RADIO CONTINUUM; STARS;

D O I：

10.1093/mnras/261.4.865

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The relation between subpulses and the total pulse intensity of four pulsars is found from observations at frequencies from 30 to 1412 MHz. The subpulses constitute a distinct component of emission, with an appreciably different distribution of sources of emission.

引用

页码：865 / 872

页数：8

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