The minimum metallicity of globular clusters and its physical origin - implications for the galaxy mass-metallicity relation and observations of proto-globular clusters at high redshift
ABSTRACT. In the local Universe, globular clusters (GCs) with metallicities [Fe/H] < −2.5 are extremely rare. In this Letter, the close connection between G
Saved in:
| Main Author: | |
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| Format: | Article (Journal) |
| Language: | English |
| Published: |
13 April 2019
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| In: |
Monthly notices of the Royal Astronomical Society. Letters
Year: 2019, Volume: 486, Issue: 1, Pages: L20-L25 |
| ISSN: | 1745-3933 |
| DOI: | 10.1093/mnrasl/slz052 |
| Online Access: | Verlag, Volltext: https://doi.org/10.1093/mnrasl/slz052 Verlag, Volltext: https://academic.oup.com/mnrasl/article/486/1/L20/5454773 
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| Author Notes: | J.M. Diederik Kruijssen |
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| 245 | 1 | 4 | |a The minimum metallicity of globular clusters and its physical origin - implications for the galaxy mass-metallicity relation and observations of proto-globular clusters at high redshift |c J.M. Diederik Kruijssen |
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| 520 | |a ABSTRACT. In the local Universe, globular clusters (GCs) with metallicities [Fe/H] < −2.5 are extremely rare. In this Letter, the close connection between G | ||
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