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Savolainen, T., Wiik, K., Valtaoja, E. and Tornikoski, M. (2008) Magnetic Field Structure in the Parsec Scale Jet of 3C 273 from Multifrequency VLBA Observations. In: Rector, T.A. and De Young, D.S., Eds., Extragalactic Jets: Theory and Observation from Radio to Gamma Ray Vol. 386 of Astronomical Society of the Pacific Conference Series, 451. (Preprint)

has been cited by the following article:

• TITLE: Classical and Relativistic Flux of Energy Conservation in Astrophysical Jets

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Galaxies: Jets Relativity

  JOURNAL NAME: Journal of High Energy Physics, Gravitation and Cosmology, Vol.2 No.1, January 7, 2016

  ABSTRACT: The conservation of the energy flux in turbulent jets which propagate in the intergalactic medium (IGM) allows deducing the law of motion in the classical and relativistic cases. Three types of IGM are considered: constant density, hyperbolic and inverse power law decrease of density. An analytical law for the evolution of the magnetic field along the radio-jets is deduced using a linear relation between the magnetic pressure and the rest density. Astrophysical applications are made to the centerline intensity of synchrotron emission in NGC315 and to the magnetic field of 3C273.