Pulsar

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Composite Optical/X-ray image of the Crab Nebula pulsar, showing surrounding nebular gases stirred by the pulsar's magnetic field and radiation.
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The Vela Pulsar, a neutron star corpse left from a titanic stellar supernova explosion, shoots through space powered by a jet emitted from one of the neutron star's rotational poles.

Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation. The radiation intensity varies at a regular period, believed to result from the rotation of the star. The pulsar was discovered in 1967, by Jocelyn Bell and Antony Hewish of the University of Cambridge, England. Initially baffled as to the unnaturally regular nature of its emissions, the pair dubbed their discovery LGM-1, for "little green men"; their pulsar was later dubbed CP 1919, and is now known as PSR 1919+21.

CP 1919 emits in radio wavelengths, but pulsars have subsequently been found to emit in the X-ray and gamma ray wavelengths. Along with four others - but not including Jocelyn Bell - Hewish received the 1974 Nobel Prize in Physics for the work.

Three distinct classes of pulsars are presently known to astronomers, according to the source of energy that powers the radiation:

Although all three classes of objects are neutron stars, their observable behaviour and the underlying physics are quite different. There are, however, connections. For example, X-ray pulsars are probably old rotation-powered pulsars that have already lost most of their energy, and have only become visible again after their binary companions expanded and began transferring matter on to the neutron star. The process of accretion can in turn transfer enough angular momentum to the neutron star to "recycle" it as a rotation-powered millisecond pulsar.

Significant pulsars

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Pulsars

See also: Pulsar, 1967, 1968, 1974, 2004, Accretion, Angular momentum, Antony Hewish, Astronomer