Rotation-powered pulsar 23715 220894782 2008-06-22T03:05:12Z SmackBot 433328 Date the maintenance tags or general fixes {{Expand|date=June 2008}} [[Image:Chandra-crab.jpg|thumb|250px|right|Composite Optical/X-ray image of the [[Crab Nebula]] pulsar, showing surrounding nebular gases stirred by the pulsar's magnetic field and radiation.]] '''Rotation-powered pulsar''' is one of the major classes of [[pulsar]]s. A Rotation-powered pulsar is a rapidly rotating [[neutron star]], whose [[electromagnetic radiation]] is observed in regularly spaced intervals, or ''pulses''. It differs from other types of [[pulsar]]s in that the source of power for the production of radiation is the loss of [[rotational energy]]. ==Name== As the first type of pulsars to be discovered, rotation-powered pulsars were originally known simply as '''pulsars''', a term coined by a [[Daily Telegraph]] journalist as a contraction of "pulsating star". Although it was soon learned that the pulses were related to rotation rather than to physical expansion and contraction, as in true [[Variable star#Pulsating variable stars|pulsating variable stars]], the term stuck. After the discovery of [[accretion (science)|accretion]]-powered [[x-ray pulsar]]s, rotation-powered pulsars were known as '''radio pulsars'''. Since rotation-powered pulsars are now known that emit [[x-ray]]s but not [[radio waves]], the term "rotation-powered pulsar" is preferred. ==Theory== There is general agreement that what we observe as a pulse is what happens when a beam of radiation points in our direction, once for every rotation of the neutron star. The origin of the beam is related to the misalignment of the rotation axis and the axis of the [[magnetic field]] of the star. The beam is emitted from the poles of the neutron star's magnetic field, which may be offset from the rotational poles by a wide angle. The source of energy of the beam is the rotational energy of the neutron star. The rotation slows down over time as the energy is emitted. [[Millisecond pulsar]]s are thought to have been spun up to high rotational speed by infalling matter pulled off a companion star. Of interest to the study of the state of the matter in a neutron stars are the ''[[Glitch (astronomy)|glitches]]'' observed in the rotation velocity of the neutron star. This velocity is decreasing slowly but steadily, except by sudden variations. One model put forward to explain these glitches is that they are the result of "starquakes" that adjust the crust of the neutron star. Models where the glitch is due to a decoupling of the possibly [[superconductivity|superconducting]] interior of the star have also been advanced. In both cases, the star's [[moment of inertia]] changes, but its [[angular momentum]] doesn't, resulting in a change in rotation rate. In [[2003]] observations of the [[Crab nebula]] pulsar's signal revealed "sub-pulses" within the main signal with durations of only nanoseconds. It is thought that these nanosecond pulses are emitted by regions on the pulsar's surface 60cm in diameter or smaller, making them the smallest structures outside the solar system to be measured. ==Importance== The discovery of pulsars allowed astronomers to study an object never observed before, the [[neutron star]]. This kind of object is the only place where the behaviour of matter at [[atomic nucleus|nuclear]] density can be observed (though not directly). Also, millisecond pulsars have allowed a test of [[general relativity]] in conditions of an intense gravitational field. ==Significant pulsars== *The first radio pulsar, [[CP 1919]] (now known as [[PSR B1919+21]]), with a pulse period of 1.337 seconds and a pulse width of 0.04 second, was discovered in [[1967]]. A drawing of this pulsar's radio waves was used as the cover of British rock band [[Joy Division]]'s debut album, "[[Unknown Pleasures]]". *The first binary pulsar, [[PSR B1913+16]], confirming general relativity and proving the existence of gravitational waves *The first millisecond pulsar, [[PSR B1937+21]] *The first pulsar with planets, [[PSR B1257+12]] *The first double pulsar binary system, [[PSR J0737-3039]] *The longest period pulsar, [[PSR J2144-3933]] ==See also== * [[Neutron star]] * [[Pulsar]] * [[Radio pulsar]] * [[X-ray pulsar]] * [[Magnetar]] * [[Millisecond pulsar]] * [[Pulsar planets]] * [[Rotating radio transient]] [[Category:Pulsars]] [[Category:Rotation-powered pulsars|*]] [[ca:Púlsar]] [[cs:Pulsar]] [[da:pulsar]] [[de:Pulsar]] [[et:Pulsar]] [[fr:Pulsar]] [[it:Pulsar]] [[nl:Pulsar]] [[ja:パルサー]] [[pl:Pulsar]] [[fi:Pulsari]] [[sv:Pulsar]] [[zh:中子星]]