A test for asymptotic giant branch evolution theories: planetary nebulae in the Large Magellanic Cloud
We used a new generation of asymptotic giant branch (AGB) stellar models that include dust formation in the stellar winds to find the links between evolutionary models and the observed properties of a homogeneous sample of Large Magellanic Cloud (LMC) planetary nebulae (PNe). Comparison between the evolutionary yields of elements such as CNO and
Ventura, P. et al.
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2015