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Planetary nebulae in the magellanic clouds

We present optical and UV observations of PNe and derive their abundancesand the implications for chemical evolution. We observe the HBB reaction andalso an oxygen depletion via the ON reaction in the more massive stars, and anoxygen production (like carbon) during the 3rd dredge-up (the e ect is ec...

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Publicat a:Revista Mexicana de Astronomía y Astrofísica
Autors principals: P. Leisy, M. Dennefeld
Format: Artigo
Idioma:Inglês
Publicat: Universidad Nacional Autónoma de México 2000
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Accés en línia:https://www.redalyc.org/articulo.oa?id=57100957
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