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Jet Collimation
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Summary
Jet Collimation
refers to the process by which
Astrophysical Jets
, typically emitted by objects like
Black Holes
or
Neutron Stars
, become narrowly focused and maintain a
Coherent Structure
over vast distances. This phenomenon is crucial for understanding the dynamics of
High-energy astrophysical environments
and the mechanisms behind
Energy transfer in the universe
.
Concepts
Astrophysical Jets
Black Holes
Neutron Stars
Magnetic Fields
Accretion Disks
Relativistic Jets
Jet Launching Mechanisms
Jet Propagation
Energy Transfer
Synchrotron Radiation
Relevant Degrees
Air and Space Transport Engineering 60%
Aerodynamics 40%
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