Ambipolar Heating of Magnetars
Magnetars, neutron stars thought to be with ultrastrong magnetic fields of 10 ^14–15 G, are observed to be much hotter than ordinary pulsars with ∼10 ^12 G, and additional heating sources are required. One possibility is heating by the ambipolar diffusion in the stellar core. This scenario is examin...
Збережено в:
| Автори: | , , , , , |
|---|---|
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2023-01-01
|
| Серія: | The Astrophysical Journal |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/1538-4357/acbd38 |
| Теги: |
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|