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NGC 1852
Expected Differences Between AGB Stars in the LMC and the SMC Due to Differences in Chemical Composition
Arxiv:1802.01597V1 [Astro-Ph.GA] 5 Feb 2018 Born 1991)
Ngc Catalogue Ngc Catalogue
Arxiv:1803.10763V1 [Astro-Ph.GA] 28 Mar 2018
19 91Apjs. . .76. .185E the Astrophysical Journal Supplement
Chemical Evolution of the Large Magellanic Cloud)
Dust-Enshrouded Giants in Clusters in the Magellanic Clouds Stellar Dust Emission Are Essential to Measure the Mass-Loss Rate from These Stars
INFRARED SURFACE BRIGHTNESS FLUCTUATIONS of MAGELLANIC STAR CLUSTERS1 Rosa A
Stars, Galaxies, and Beyond, 2012
Statistical Analyses of Massive Stars and Stellar Populations
Catalogue of Large Magellanic Cloud Star Clusters Observed in the Washington Photometric System