What type of astronomical object is mainly observed in Perseus A?

Perseus A, also known as NGC 1275, is a prominent active galaxy located in the Perseus cluster of galaxies. The key feature of Perseus A is its central supermassive black hole, which is the dominant force driving the various energetic phenomena observed in the galaxy.

The presence of the supermassive black hole at the center of Perseus A is evident through the observation of high-energy emissions, including X-rays, which arise due to the accretion of matter onto the black hole. This matter forms an accretion disk, radiating energy as it spirals inward and heats up due to gravitational and frictional forces. Additionally, jets of relativistic particles can be seen emanating from the supermassive black hole, further indicating its presence and activity.

By contrast, objects like neutron stars, white dwarfs, and pulsars represent different stages or types of stellar evolution. Neutron stars are the remnants of massive stars after supernova explosions but are not found in the center of galaxies like Perseus A. White dwarfs are similar remnants of less massive stars and typically do not exhibit the same high-energy phenomena associated with active galactic nuclei. Pulsars are rotating neutron stars that emit beams of radiation;