Shaping of elliptical planetary nebulae - The influence of dust-driven winds of AGB stars

Shaping of elliptical planetary nebulae - The influence of dust-driven winds of AGB stars

We calculated a model to investigate the shaping of a PN morphological group, i.e. elliptical PNe, in terms of the so-called Interacting Winds Model. The angle-dependent mass loss generated by a dust driven wind due to a slow rotation of the AGE star is a

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Veröffentlicht in:Astronomy and astrophysics (Berlin) 2000, Vol.354 (2), p.573
Hauptverfasser: Reimers, C, Dorfi, EA, Höfner, S
Format: Artikel
Sprache:eng
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Zusammenfassung:We calculated a model to investigate the shaping of a PN morphological group, i.e. elliptical PNe, in terms of the so-called Interacting Winds Model. The angle-dependent mass loss generated by a dust driven wind due to a slow rotation of the AGE star is a
ISSN:0004-6361