Neutron star dynamics, braking indices and energy dissipation

被引：8

作者：

Alpar, MA ^{[1
]}

机构：

[1] Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey

来源：

SPACE BASED ASTRONOMY: ISO, AGN, RADIOPULSARS AND THE SUN | 1998年 / 21卷 / 1-2期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1016/S0273-1177(97)00800-4

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

Models of pulsar glitches and postglich relaxation are reviewed. Implications for braking indices due to internal torques in the neutron star, and energy dissipation by internal torques are discussed. AU recent observations of pulsars with large (Vela pulsar like) glitches and second derivatives are seen to fit with the same glitch dynamics that the Vela pulsar exhibits. (C)1998 COSPAR. Published by Elsevier Science Ltd.

引用

页码：159 / 166

页数：8

共 19 条

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