THE INFLUENCE OF INCLINATION ANGLE ON POLAR CAP HEATING OF J0901-4046 RADIOPULSAR
Аннотация и ключевые слова
Аннотация (русский):
The influence of inclination angle to electron-positron pairs production in inner gap and polar cap heating by reverse positron current in case of J0901-4046 radiopulsar is considered. It is shown that J0901-4046 pulsar ``work" may be explained by the presence of a highly curved small scale surface magnetic field without the substantial increasing of its dipolar magnetic field at inclination angle values $\chi \lesssim 30^{\circ}$.

Ключевые слова:
pulsars: general, individual (J0901-4046)
Список литературы

1. Barsukov D., Morozov I., and Popov A., 2023, Astronomy Letters, 49, p. 806

2. Beskin V. and Istomin A., 2022, Monthly Notices of the Royal Astronomical Society, 516, p. 5084

3. Caleb M., Heywood I., Rajwade K., et al., 2022, Nature Astronomy, 6, p. 828

4. Kantor E. and Tsygan A., 2003, Astronomy Reports, 47, p. 613

5. Malov I. and Nikitina E., 2011, Astronomy Reports, 55, p. 878

6. Manchester R., Hobbs G., Teoh A., et al., 2005, The Astronomical Journal, 129, p. 1993

7. Rankin J., 1990, Astrophysical Journal, 352, p. 247

8. Sob'yanin D., 2023, Physical Review D, 107, id. L081301.

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