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- W1617445937 abstract "Abstract It is assumed that the acceleration and collimation mechanisms of jets are the same in all the classes of astrophysical objects which are observed to produce jets. These classes now include: active galactic nuclei, young stellar objects, massive x-ray binaries, low mass x-ray binaries, black hole x-ray transients, symbiotic systems, planetary nebulae, and supersoft x-ray sources. On the basis of this assumption, an attempt is made, to identify the necessary ingredients for the acceleration and collimation mechanism. It is argued that: (i) jets are produced at the center of accretion disks which are threaded by a vertical magnetic field, (ii) the production of powerful jets requires, in addition, an energy/wind source associated with the central object. Tentative explanations for the presence of jets in some classes of objects and absence in others are given. Some critical observation that can test the ideas presented in this paper are suggested." @default.
- W1617445937 created "2016-06-24" @default.
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- W1617445937 date "1997-01-01" @default.
- W1617445937 modified "2023-10-18" @default.
- W1617445937 title "The Formation of Astrophysical Jets" @default.
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- W1617445937 doi "https://doi.org/10.1017/s0252921100044298" @default.
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