Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud

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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Bibliographic Details
Main Author: Asa'd, Randa (author)
Other Authors: Hernandez, S. (author), As’ad, A. M. (author), Molero, M. (author), Matteucci, F. (author), Larsen, S. (author), Chilingarian, Igor V. (author)
Format: article
Published: 2022
Subjects:
Galaxy chemical evolution (580)
Star clusters (1567)
Large Magellanic Cloud (903)
Online Access:http://hdl.handle.net/11073/23591
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http://hdl.handle.net/11073/23591

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