On the Evolution of Angles between the Magnetic Moment and the Axis of Rotation in Radio Pulsars

封面

如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

Three methods were used to calculate the angles β between the magnetic moment and the axis of rotation of central neutron stars for 307 known radio pulsars. There is no explicit statistical dependence of the calculated angles β on the kinematic age of pulsars. It follows from this that either the indicated angle does not change noticeably with the age of the pulsar, or pulsars are born with an arbitrary inclination angle.

作者简介

I. Malov

P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Pushchino Radio Astronomy Observatory named after V. V. Vitkevich, Astrospace Center

Email: malov@prao.ru
Pushchino, Russia

O. Malov

P.N. Lebedev Physical Institute of the Russian Academy of Sciences, Pushchino Radio Astronomy Observatory named after V. V. Vitkevich, Astrospace Center

编辑信件的主要联系方式.
Email: malov@prao.ru
Pushchino, Russia

参考

  1. L. Davis and M. Goldstein, Astrophys. J. 159, L81 (1970).
  2. В. С. Бескин, A. В. Гуревич, Я. Н. Истомин, ЖЭТФ 85 (2), 401 (1983).
  3. A. Philippov, A. Tchekhovskoy, and J. G. Li, Monthly Not. Roy. Astron. Soc. 441, 1879 (2014).
  4. Р. Манчестер, Дж.Тейлор, Пульсары (М: Мир, 1980).
  5. R. N. Manchester, G. B. Hobbs, A. Teoh, and M. Hobbs, Astron. J. 129, 1993 (2005).
  6. I. F. Malov, Monthly Not. Roy. Astron. Soc. 502, 809 (2021).
  7. И. Ф. Малов, О. И. Малов, Астрон. журн. 83 (6), 542 (2006).
  8. S. V. Bogovalov, Astron. and Astrophys. 349, 1017 (1999).

补充文件

附件文件
动作
1. JATS XML
下载
2.

下载 (114KB)
索引源数据
3.

下载 (45KB)
索引源数据
4.

下载 (44KB)
索引源数据
5.

下载 (28KB)
索引源数据

版权所有 © И.Ф. Малов, О.И. Малов, 2023