For constant-density surroundings, energy-flux conservation gives jet length growing as t^(3/5) and velocity decaying as x^(-2/3); the same method is extended to other density profiles and to 3C31 synchrotron emission fits.
V ., Suzuki-Vidal, F., Ciardi, A., et al., Laboratory simulations of astrophysical jets, in: Bonanno, A., de Gouveia Dal Pino, E., & Koso- vichev, A
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Conservation of the Flux of Energy in Extra-Galactic Jets
For constant-density surroundings, energy-flux conservation gives jet length growing as t^(3/5) and velocity decaying as x^(-2/3); the same method is extended to other density profiles and to 3C31 synchrotron emission fits.