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MHD equilibria of Helical Jets
Published online by Cambridge University Press: 25 May 2016
Extract
From recent high angular resolution (≃ 0.1 arcsec) observations of some extragalactic jets (in particular we refer to the radio, optical, and ultraviolet images of the M 87 jet, of 3C 66B, and 3C 264) it can be inferred that the synchrotron emission from the jet comes mainly from an external, quasi-cylindrical surface on which bright helical filamentary structures can be clearly recognized.
- Type
- Radio Source Modelling and Emission Mechanisms
- Information
- Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 457 - 458
- Copyright
- Copyright © Kluwer 1996