The evolution of gas-phase metallicity and resolved abundances in star-forming galaxies at z ≈ 0.6 – 1.8
We present an analysis of the chemical abundance properties of ≈650 star-forming galaxies at z ≈ 0.6 – 1.8. Using integral-field observations from the K - band Multi-Object Spectrograph (KMOS), we quantify the [N II]/Hα emission-line ratio, a proxy for the gas-phase Oxygen abundance within the inter...
| Main Authors: | , , , , , , , , , , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
Oxford University Press
2020
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