Dynamo-Driven Outflows in Pre-Planetary Nebulae
@article{Blackman2003DynamoDrivenOI, title={Dynamo-Driven Outflows in Pre-Planetary Nebulae}, author={E. Blackman}, journal={arXiv: Astrophysics}, year={2003} }
The plethora of asymmetric planetary nebulae and the curiously high momenta of pre-planetary nebula outflows suggest that rotational energy is extracted from the engines. Magneto-rotational outflows driven by dynamos might be operating therein. I summarize scenarios involving (a) an isolated AGB star and (b) a binary. The efficacy of (a) requires re-establishing differential rotation over the AGB star's lifetime, whereas (b) delivers the angular momentum at the end of the AGB phase when needed… CONTINUE READING
References
SHOWING 1-7 OF 7 REFERENCES
Origin and Evolution of Planetary Nebulae (Cambridge: CUP
- 2000
ApJ
- ApJ
- 1998
Differential rotation and stellar convection (Berlin: Verlag
- 1989
Proc. of the workshop on " Magnetic Fields and Star Formation " Madrid, 2003 (Dodrehcht: Kluwer) eds. A.I. Gómez de Castro et al
- Proc. of the workshop on " Magnetic Fields and Star Formation " Madrid, 2003 (Dodrehcht: Kluwer) eds. A.I. Gómez de Castro et al