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Classical and relativistic conservation of momentum flux in radio-galaxies | | L. Zaninetti
; | | Date: |
3 Aug 2015 | | Abstract: | A new set of laws of motion for turbulent jets propagating in an
intergalactic medium characterized by a decreasing density is derived by
applying conservation of momentum flux both in the classical and relativistic
framework. Two characteristic features of radio-galaxies, such as oscillations
and curvature, are modeled by a classical helicoidal jet. A third feature of a
radio-galaxy, the appearance of knots, is explained as an effect due to the
theory of images. | | Source: | arXiv, 1508.0360 | | Services: | Forum | Review | PDF | Favorites | |
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