z-logo
open-access-imgOpen Access
Using the Age and Metallicity of 8 Star Clusters to confirm the Chemical Enrichment History of the LMC
Author(s) -
Farah Balaha,
Maryam Alhosani,
Randa Asa’d,
I. Chillingarian
Publication year - 2019
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1258/1/012020
Subject(s) - metallicity , large magellanic cloud , galaxy , astrophysics , star (game theory) , physics , star cluster , star formation , astronomy
In this paper, we find the ages and metallicities of 8 Large Magellanic Cloud (LMC) star clusters obtained from integrated light spectra and use them to obtain the Chemical Enrichment History of the host galaxy. Our results are in good agreement with those obtained from resolved studies. This confirms that this method can be used for far away galaxies for which their star clusters are not resolved.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here