ON THE TIMING HISTORY OF PSR B1509-58

被引：9

作者：

BLANDFORD, RD

机构：

[1] California Institute of Technology, Theoretical Astrophysics, 130-33, Pasadena, 91125, CA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1994年 / 267卷 / 01期

关键词：

MHD; STARS; MAGNETIC FIELDS; PULSARS; GENERAL; INDIVIDUAL; B1509-58;

D O I：

10.1093/mnras/267.1.L7

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The measurement of the third frequency derivative of PSR B1509 - 58 reported by Kaspi et al. is consistent with a constant magnetic moment. If a more accurate, stable measurement can be made. it should be possible to test directly models in which the magnetic moment varies.

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页码：L7 / L8

页数：2

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