Pulsars are neutron stars that emit radiation through their magnetic poles due to their high spin and strong electromagnetic fields, which focus the radiation outward. The alignment of the magnetic and rotational poles can differ, causing the emitted beam to sweep around like a searchlight. Quasars, on the other hand, produce visible radiation from matter that collides at high energy as it falls toward a black hole, before crossing the event horizon. This process allows us to observe the energy released, despite the common belief that nothing escapes a black hole. Understanding these phenomena highlights the complex interactions between gravity, magnetism, and radiation in astrophysics.