Atmospheric Mass Loss from TOI-1259 A b, a Gas Giant Planet with a White Dwarf Companion
The lack of close-in Neptune-mass exoplanets evident in transit surveys has largely been attributed to either photoevaporative mass loss or high-eccentricity migration. To distinguish between these two possibilities, we investigate the origins of TOI-1259 A b, a Saturn-mass (0.4 M _J , 1.0 R _J ) ex...
Збережено в:
| Автори: | , , , , , , , , |
|---|---|
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2025-01-01
|
| Серія: | The Astronomical Journal |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/1538-3881/ada49f |
| Теги: |
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|