The Low-mass Stellar Initial Mass Function in Nearby Ultrafaint Dwarf Galaxies
The stellar initial mass function (IMF) describes the distribution of stellar masses that form in a given star formation event. The long main-sequence lifetimes of low-mass stars mean that the IMF in this regime (below ∼ 1 M _⊙ ) can be investigated through star counts. Ultrafaint dwarf galaxies are...
Сохранить в:
| Главные авторы: | , , , , , |
|---|---|
| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
IOP Publishing
2024-01-01
|
| Серии: | The Astrophysical Journal |
| Предметы: | |
| Online-ссылка: | https://doi.org/10.3847/1538-4357/ad4020 |
| Метки: |
Нет меток, Требуется 1-ая метка записи!
|