Applying the empirical abundance method to simulated observations of NGC 3132 from a 3D model overestimates the input oxygen abundance by up to 35% due to line-of-sight projection effects.
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Dissecting NGC 3132: Tracing the mass-loss history of the southern ring planetary nebula
Applying the empirical abundance method to simulated observations of NGC 3132 from a 3D model overestimates the input oxygen abundance by up to 35% due to line-of-sight projection effects.