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
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| Main Author: | |
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| Format: | Article (Journal) |
| Language: | English |
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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 |
| Summary: | 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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| Item Description: | Gesehen am 04.06.2019 |
| Physical Description: | Online Resource |
| ISSN: | 1745-3933 |
| DOI: | 10.1093/mnrasl/slz052 |