Massive Star Formation in Metal-Enriched Haloes at High Redshift
The formation of supermassive stars has generally been studied under the assumption of rapid accretion of pristine metal-free gas. Recently it was found, however, that gas enriched to metallicities up to $Z \sim 10^{-3}$ Z$_{\odot}$ can also facilitate supermassive star formation, as long as the tot...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Maynooth Academic Publishing
2020-08-01
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| Series: | The Open Journal of Astrophysics |
| Online Access: | https://doi.org/10.21105/astro.2006.14625 |