Influence of a Small-Scale Magnetic Field on the Heating of the Polar Cap of the Radio Pulsar J0901–4046
- Авторлар: Barsukov D.1, Morozov I.1, Popov A.1
-
Мекемелер:
- Ioffe Physical–Technical Institute, Russian Academy of Sciences
- Шығарылым: Том 49, № 12 (2023)
- Беттер: 869-874
- Бөлім: Articles
- URL: https://journals.rcsi.science/0320-0108/article/view/254246
- DOI: https://doi.org/10.31857/S032001082312001X
- EDN: https://elibrary.ru/RXHJMW
- ID: 254246
Дәйексөз келтіру
Аннотация
The pulsar J0901–4046 has a spin periodP = 75.8 s and is themost slowly rotating one among
the isolated radio pulsars. We have considered the influence of a small-scale magnetic field in the offcentered
dipole model on the polar cap heating by the reverse positron current in the inner gap of the pulsar.
We have assumed that the electron–positron pairs in the gap are created in bound states, which then are
broken by thermal photons from the stellar surface.
Негізгі сөздер
Авторлар туралы
D. Barsukov
Ioffe Physical–Technical Institute, Russian Academy of Sciences
Email: bars.astro@mail.ioffe.ru
St. Petersburg, 194021 Russia
I. Morozov
Ioffe Physical–Technical Institute, Russian Academy of Sciences
Email: bars.astro@mail.ioffe.ru
St. Petersburg, 194021 Russia
A. Popov
Ioffe Physical–Technical Institute, Russian Academy of Sciences
Хат алмасуға жауапты Автор.
Email: bars.astro@mail.ioffe.ru
St. Petersburg, 194021 Russia
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