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A mechanism for the production of jets and Ansae in Planetary Nebulae

Published online by Cambridge University Press:  25 May 2016

Adam Frank ,
Bruce Balick  and
Mario Livio
Adam Frank
Affiliation:
1 Department of Physics & Astronomy, Univ. Rochester
Bruce Balick
Affiliation:
2Astronomy Department, Univ. of Washington
Mario Livio
Affiliation:
3Space Telescope Science Institute

Extract

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The general properties of elliptical planetary nebulae have been very successfully explained by a class of hydrodynamic models known as interacting stellar winds (ISW). PNs also contain a variety of microstructures (Anase,“FLIERs”) whose origins have remained puzzling. We (Frank, Balick, & Livio 1996) have shown that such flows will naturally occur in the ISW model in momentum-conserving PPN bubbles, and that they can naturally account for the formation of jets and ansae in a way consistent with extant observations.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 225
Copyright
Copyright © Kluwer 1997 

References

Canto, J., Tenorio-Tagle, G., & Rozyczka, M. 1988. A&A 192 287.Google Scholar
Kahn, F.D., & Breitschwert, D. 1990, MNRAS 242 505.CrossRefGoogle Scholar
Frank, A., Balick, B., & Livio, M., 1996, ApJ, 471, L53.CrossRefGoogle Scholar