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NGC 6826: A UNIFIED STUDY OF THE PLANETARY NEBULA AND ITS CENTRAL STARS

We present a methodology to obtain a stellar-nebular self-consistent model. Distance is determined using theoretical evolutive tracks of central stars of planetary nebulae. This methodology is applied to study of the galactic planetary nebula NGC 6826. A unified model requieres more work, but its un...

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書誌詳細
出版年:Revista Mexicana de Astronomía y Astrofísica
主要な著者: C. R. Fierro, A. Peimbert, L. Georgiev, C. Morisset, A. Arrieta
フォーマット: Artigo
言語:Inglês
出版事項: Universidad Nacional Autónoma de México 2011
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オンライン・アクセス:https://www.redalyc.org/articulo.oa?id=57121297084
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