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Is the Jet in M87 Magnetically Confined?
Published online by Cambridge University Press: 04 August 2017
Abstract
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Calculations of the minimum pressure in the M87 jet show that the jet pressure is an order of magnitude in excess of the thermal pressure in the interstellar medium calculated from the X-ray emission. The continuous energy input required to produce the jet emission is incompatible with a freely expanding jet. On the other hand, the uniform jet expansion, the jet emission and the jet polarization can be explained if the jet is self-confined by j x B forces.
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- Session VI
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- Copyright © Reidel 1985
References
Begelman, M.C.
1982, in IAU Symposium 97, Extragalactic Radio Sources, ed. Heeschen, D.S. and Wade, CM. (Dordrecht: Reidel).Google Scholar
Ferrari, A.
1985, in IAU Symposium 107, Unstable Current Systems and Plasma Instabilities in Astrophysics, ed. Kundu, M. and Holman, G. (Dordrecht: Reidel)(this volume).Google Scholar
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