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disks are a ubiquitous phenomenon in astrophysics; active galactic nuclei, protoplanetary
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astrophysical jet is an astronomical phenomenon where outflows of ionised matter are emitted as an extended beam along the axis of rotation. When this greatly accelerated matter in the beam approaches the speed of light,
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Disks† Gennaro D’Angelo1 School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, United Kingdom NASA-ARC, Space Science and Astrobiology Division, MS 245-3, Moffett Field, CA 94035, USA gdangelo@arc.nasa.gov and Stephen H. Lubow Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA lubow@stsci.edu …
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