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Stagnation knots in planetary nebulae

We present an alternative model for the formation of fast low-ionization emission regions (FLIERs) in planetarynebulae. In this model, a concave bow-shock structure is formed as a result of a reduced momentum ow alongthe symmetry axis of a stellar wind. FLIERS are formed from the shocked ambient med...

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Publié dans:Revista Mexicana de Astronomía y Astrofísica
Auteurs principaux: J. A. López, A. J. Lim, W. Steffen
Format: Artigo
Langue:Inglês
Publié: Universidad Nacional Autónoma de México 2002
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Accès en ligne:https://www.redalyc.org/articulo.oa?id=57112052
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