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•A hidden verification in binary systems Pulsars, or neutron stars, are highly magnetized and rotating neutron stars that emit electromagnetic radiation from their magnetic poles. These objects become very useful tools for astronomers due to their extremely regular cycles, which range from milliseconds to seconds. This regularity makes pulsars a natural tool for observation.
There are three different classes of pulsars, classified according to the source of their electromagnetic radiation: spinning pulsars, accumulation pulsars, and magnetars. All of these are neutron stars, but their observable behavior and underlying physics are quite different.
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