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...
Furkejuvvon:
| Váldodahkkit: | , , , , , |
|---|---|
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
IOP Publishing
2024-01-01
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| Ráidu: | The Astrophysical Journal |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.3847/1538-4357/ad4020 |
| Fáddágilkorat: |
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