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Cyclotron Radiation: a Jet-Driving Mechanism in Magnetized PN Nuclei

Published online by Cambridge University Press:  26 May 2016

A. V. Serber
A. V. Serber*
Affiliation:
Institute of Applied Physics of the Russian Academy of Sciences, 46 Ulyanov st., 603950 Nizhny Novgorod, Russia

Abstract

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We claim that cyclotron radiation at the electron gyrofrequency ωB is an efficient mechanism capable of driving highly collimated bipolar jets in magnetized nuclei of planetary nebulae.

Type
Part VII: Nebular Morphology and Dynamics
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 465 - 466
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Lamers, H. J. G. L. M., & Cassinelli, J. P. 1999, Introduction to Stellar Winds (Cambridge University Press)CrossRefGoogle Scholar
Wickramasinghe, D.T., & Ferrario, L. 2000, PASP, 112, 873 Google Scholar
Zheleznyakov, V. V. 1996, Radiation in Astrophysical Plasmas (Kluwer)Google Scholar
Zheleznyakov, V. V., Serber, A. V., & Kuijpers, J. 1996, A&A, 308, 465 Google Scholar