Radio astronomy uses radio telescopes and receivers to capture radio waves emitted by astronomical objects like stars, galaxies, and nebulae. Radio telescopes work similarly to optical telescopes but detect radio waves rather than visible light. They capture radio emissions that can reveal information about phenomena like cold molecular clouds, strong magnetic fields, and relativistic electrons. Radio astronomy allows observation of regions that are obscured at optical wavelengths. Interferometry combines signals from multiple telescopes to achieve higher resolution. Common radio sources observed include galaxies, nebulae, stars, and active regions in our own and other galaxies.