radio source
A radio source appears as a bright point on the astronomer's computer screen.
Noun: An astronomical object that emits significant amounts of electromagnetic radiation in the radio frequency range of the spectrum. It is a celestial body or region detectable by radio telescopes.
The term "radio source" is used in astronomy and astrophysics to identify and classify objects in space based on their radio wave emissions. It is a neutral, technical descriptor.
Examples: * The astronomer identified a new radio source in the distant galaxy. * Pulsars and quasars are among the most powerful known radio sources. * The map of the sky shows the location of several strong radio sources.
- Extended vs. Compact Radio Source: Used to describe the physical size of the emitting region as observed from Earth. An extended source appears spread out, while a compact source appears point-like.
- Radio Source Catalog: Refers to formal astronomical catalogs, such as the Third Cambridge Catalogue (3C), which list and number identified radio sources (e.g., 3C 273 is a famous quasar).
- Radio Astronomy (n): The branch of astronomy that studies celestial objects by observing their radio frequency emissions.
- Radio Telescope (n): An instrument used to detect and collect radio waves from space.
- Radio Galaxy (n): A specific type of galaxy that is an exceptionally powerful radio source.
- Radio emitter (n): A less common but direct synonym.
- Celestial radio emitter (n): A more descriptive synonym emphasizing the astronomical context.
- Background Radio Source: Refers to the cumulative, diffuse radio emission from many distant, unresolved sources.
- Variable Radio Source: A radio source whose observed intensity changes over time.
- Radio-loud: An adjective used to describe active galactic nuclei (like quasars) that are strong radio sources, as opposed to "radio-quiet" ones.
A radio source appears as a bright point on the astronomer's computer screen.
- an object that radiates radio waves