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

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Resumo

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.

Sobre autores

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

Autor responsável pela correspondência
Email: malov@prao.ru
Pushchino, Russia

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Declaração de direitos autorais © И.Ф. Малов, О.И. Малов, 2023