JWST’s First Glimpse of a z > 2 Forming Cluster Reveals a Top-heavy Stellar Mass Function
Clusters and their progenitors (protoclusters) at z ∼ 2 − 4, the peak epoch of star formation, are ideal laboratories to study the formation process of both the clusters themselves and their member galaxies. However, a complete census of their member galaxies has been challenging due to observationa...
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| Huvudupphov: | , , , , , , , , , , , , , |
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| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
IOP Publishing
2024-01-01
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| Serie: | The Astrophysical Journal Letters |
| Ämnen: | |
| Länkar: | https://doi.org/10.3847/2041-8213/ad4986 |
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