The SAMI Galaxy Survey: the link between [α/Fe] and kinematic morphology
We explore a sample of 1492 galaxies with measurements of the mean stellar population properties and the spin parameter proxy, lambda(Re), drawn from the SAMI Galaxy Survey. We fit a global [alpha/Fe]-sigma relation, finding that [alpha/Fe] = (0.395 +/- 0.010)log(10)(sigma) - (0.627 +/- 0.002). We o...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Main Authors: | , , , , , , , , , , , , , , , , , , |
Other Authors: | |
Format: | Article in Journal/Newspaper |
Language: | unknown |
Published: |
Oxford University Press (OUP)
2022
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Subjects: | |
Online Access: | http://hdl.handle.net/1959.3/467472 https://doi.org/10.1093/mnras/stac1221 |