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GAVRT detects the radio emission generated by the jet, which emerges from the interaction between the accretion disk and the supermassive black hole.

Key Terms and Concepts: 
 
  • Quasars: Extremely bright and distant objects powered by supermassive black holes.
  • Radio Emissions: Electromagnetic waves emitted by astronomical objects, crucial for studying black holes and quasars.
  • Magnetic Fields: Regions around black holes where magnetic forces are strong, influencing the behavior of jets and emissions.
  • Interstellar Medium: The matter that exists in the space between stars, affecting the propagation of radio waves from quasars.
 
 
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