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Acceleration of Relativistic Particles in Stellar Jets
1993A model is presented that can account for the nonthermal emission seen in some Young Stellar Objects. The relativistic electrons producing the synchrotron radiation can be accelerated at the (collisionless) bow shocks or termination shocks that are formed when jets from the central object propagate into the molecular cloud.
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A Review on Multiphase Underwater Jets and Plumes: Droplets, Hydrodynamics, and Chemistry
Reviews of Geophysics, 2020Michel C Boufadel +2 more
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Internal gravity waves from atmospheric jets and fronts
Reviews of Geophysics, 2014Riwal Plougonven, Fuqing Zhang
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Relativistic Jets from Active Galactic Nuclei
Annual Review of Astronomy and Astrophysics, 2019R D Blandford
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Particle acceleration in astrophysical jets
New Astronomy Reviews, 2020James H Matthews, Katherine M Blundell
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Molecular jets from low-mass young protostellar objects
Astronomy and Astrophysics Review, 2020Chin-Fei Lee 李景輝
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Very-high-energy particle acceleration powered by the jets of the microquasar SS 433
Nature, 2018A U Abeysekara, S Y Benzvi, T Capistrán
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