Pulsar beams - Conal not patchy

被引：24

作者：

Gil, J

Krawczyk, A

机构：

[1] Astronomy Centre, Pedagogical University, 65-265 Zielona Gora

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1996年 / 280卷 / 01期

关键词：

pulsars; general; individual; PSR; 1133+16; 0320+39; 2016+28;

D O I：

10.1093/mnras/280.1.143

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We analyse the frequency dependence of pulsar characteristics and conclude that, within the angular beaming model of pulsar radiation modulation, the longitudes of subpulses should be weakly dependent on frequency as compared with the longitudes of profile components. This is actually observed in pulsars. Based on this conclusion, we argue that the structure of mean pulsar beams is conal and not patchy.

引用

页码：143 / 148

页数：6

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