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Shaping of planetary nebulae by dust driven AGB winds
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2000 (English)In: ASTROPHYSICS AND SPACE SCIENCE, ISSN 0004-640X, Vol. 272, no 1-3, 205-212 p.Article in journal (Refereed) Published
Abstract [en]

We have investigated the interacting winds model (IWM) in which the shapes of elliptical Planetary Nebulae (PNe) can be explained by the asymmetric mass loss produced by a rotating AGB star. The mass loss mechanism is based on a dust driven wind calculate

Place, publisher, year, edition, pages
KLUWER ACADEMIC PUBL , 2000. Vol. 272, no 1-3, 205-212 p.
Keyword [en]
STARS
Identifiers
URN: urn:nbn:se:uu:diva-36658OAI: oai:DiVA.org:uu-36658DiVA: diva2:64557
Note
Addresses: Reimers C, Univ Vienna, Inst Astron, Turkenschanzstr 17, A-1180 Vienna, Austria. Univ Vienna, Inst Astron, A-1180 Vienna, Austria. Univ Uppsala, Astron Observ, SE-75120 Uppsala, Sweden.Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-14

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