Radiogalaxie
A radiogalaxie is a Galaxie where a significant part of energy is not emitted by the component normal of a galaxy: star S, dust and interstellar gas. This energy, which depends on the type of radiogalaxie, can be emitted through broad a electromagnetic spectrum: as in the Infra-red , Microwave, UV, x-rays and the rays γ.
The theoretical standard model proposes that energy is generated by the matter collapse on itself to form a supermassif Black hole between 106 and 108 solar mass.
See too
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