The thermal form of this effect can occur in cluster radio halo sources due to the presence of highl
The thermal form of this effect can occur in cluster radio halo sources due to the presence of highly relativistic electrons and in the non-relativistic limit it can be described by the Kompaneets equation. It is redshift-independent and occurs through the Thomson (*) scattering of photons as they interact with thermal electrons in galaxy clusters and other reservoirs of plasma. For 10 points, name this astronomical effect that results in an alteration of the apparent brightness of the CMBR.
The thermal form of this effect can occur in cluster radio halo sources due to the presence of highly relativistic electrons and in the non-relativistic limit it can be described by the Kompaneets equation.
{Sunyaev}-{Zeldovich} effect