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- W2806160614 abstract "Photoionized nebulae comprise basically HII regions and planetary nebulae, and their abundances give important clues on the nucleosynthesis and chemical evolution of their host galaxies. There is presently a large amount of data on these objects, especially for the elements He and N, which are strongly affected by the evolution of intermediate mass stars, as well as O, Ne, S, and Ar, which are essentially synthesized in stars with larger masses. The abundances of these elements in several systems in the Local Group are discussed on the basis of distance-independent correlations." @default.
- W2806160614 created "2018-06-13" @default.
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- W2806160614 date "2016-12-14" @default.
- W2806160614 modified "2023-09-27" @default.
- W2806160614 title "Chemical abundances of photoionized nebulae in the Local Group" @default.
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- W2806160614 hasPublicationYear "2016" @default.
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