Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud
We derive the first detailed chemical abundances of three star clusters in the Large Magellanic Cloud (LMC), NGC 1831 (436 ± 22 Myr), NGC 1856 (350 ± 18 Myr), and [SL63]268 (1230 ± 62 Myr) using integrated-light spectroscopic observations obtained with the Magellan Echelle spectrograph on Magellan B...
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| Other Authors: | , , , , , |
| Format: | article |
| Published: |
2022
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| Online Access: | http://hdl.handle.net/11073/23591 |
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