Centimeter continuum emission refers to the radio emission at wavelengths of approximately 1-10 centimeters, which is a part of the electromagnetic spectrum. It is typically produced by thermal radiation from ionized gas or dust particles in astronomical objects.
Centimeter continuum emission is caused by thermal radiation from ionized gas or dust particles in astronomical objects. The atoms or molecules in these objects are excited and emit radiation as they cool down.
Centimeter continuum emission can provide information about the temperature, density, and composition of astronomical objects. It can also help us study the magnetic fields and dynamics of these objects.
Centimeter continuum emission is observed using radio telescopes, which are designed to detect radio waves from space. These telescopes are typically large and can be located on the ground or in space.
Some examples of astronomical objects that emit centimeter continuum emission include stars, galaxies, supernova remnants, and molecular clouds. This type of emission can also be observed from the cosmic microwave background radiation, which is the remnant radiation from the Big Bang.