Is Earendel a Star Cluster?: Metal-poor Globular Cluster Progenitors at z ∼ 6
The strongly lensed z ∼ 6 Sunrise galaxy offers an incredible opportunity to investigate star formation in the early Universe on parsec or smaller scales. The highly magnified object Earendel within the Sunrise was previously identified as a candidate star or binary owing to size constraints placed...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal Letters |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/2041-8213/aded93 |
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| Summary: | The strongly lensed z ∼ 6 Sunrise galaxy offers an incredible opportunity to investigate star formation in the early Universe on parsec or smaller scales. The highly magnified object Earendel within the Sunrise was previously identified as a candidate star or binary owing to size constraints placed by the lensing magnification; however, recent works have suggested that this constraint may be relaxed to even the size of star clusters. Here we explore the hypothesis that Earendel may actually be a star cluster, and we simultaneously evaluate other star clusters within the host galaxy. Leveraging deep, archival James Webb Space Telescope NIRSpec PRISM spectroscopy, we determine a spectroscopic redshift for the Sunrise galaxy z = 5.926 ± 0.013, and we fit simple stellar population (SSP) models from three premier libraries to evaluate the physical parameters of Earendel and another distinct star cluster in the Sunrise dubbed “1 b. ” We find the rest-UV through optical continuum of Earendel to be well described by an SSP, nearly equivalently to 1 b , which is confidently a star cluster. We infer that they have intermediate ages t _age ∼ 30–150 Myr, are metal-poor ( Z _⋆ ≲ 0.1 Z _⊙ ), and are consistent with the formation age–metallicity trend seen in local globular clusters. Such intermediate-age clusters are seldom probed spectroscopically in the high-redshift Universe, and we explore the extent to which these clusters can be characterized via the spectroscopic continuum. |
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| ISSN: | 2041-8205 |