The Five-hundred-meter Aperture Spherical radio Telescope (FAST) was used to study the emission properties of three long-period pulsars: PSR J1945+1211, PSR J2323+1214, and PSR J1900−0134.

They changed the name of the signal from LGM to CP, for Cambridge pulsar. Many more pulsars have been found since the first. They are believed to be rapidly rotating neutron stars with intense ...

The starburst-like diagram is called a pulsar map, because it shows the location of our sun relative to known pulsars. Pulsars are the rapidly spinning remains of dying stars—the leftover cores ...

An extremely slow pulsar has made scientists “slow down” their assumptions about other pulsars. The pace could be caused by a flashing magnetic field rather than pulsar rotation alone.

Be stars also show excess in Infrared (IR) emission. X-Ray Pulsars are magnetized Neutron Stars. In Binary systems, when the Neutron Star enters the accretion regime, it starts to accrete matter from ...

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Neutron stars are so named because in the simplest of models they are made of neutrons. They form when the core of a large star collapses, and the weight of gravity causes atoms to collapse.