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• W2123762743 startingPage "A118" @default.
• W2123762743 abstract "Aims. Chemical evolution models are useful for understanding the formation and evolution of stars and galaxies. Model predictions will be more robust when more observational constraints are used. We present chemical evolution models for the dwarf irregular galaxy NGC 6822 using chemical abundances of old and young planetary nebulae (PNe) and H ii regions as observational constraints. We use two sets of chemical abundances, one derived from collisionally excited lines (CELs) and one from recombination lines (RLs). We use our models as a tool to distinguish between both procedures for abundance determinations." @default.
• W2123762743 created "2016-06-24" @default.
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• W2123762743 date "2011-11-01" @default.
• W2123762743 modified "2023-09-30" @default.
• W2123762743 title "Planetary nebulae as observational constraints in chemical evolution models for NGC 6822" @default.
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• W2123762743 doi "https://doi.org/10.1051/0004-6361/201116957" @default.
• W2123762743 hasPublicationYear "2011" @default.
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