Pulsar


Composite Optical/X-ray image of the [[Crab Nebula pulsar, showing surrounding nebular gases stirred by the pulsar's magnetic field and radiation.]] Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation. The radiation is observed to consist of a regular series of pulses, believed to be in synchrony with the rotation of the star. Astronomers classify pulsars according to the source of energy that powers the emission of radiation. There are three presently accepted classes: 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 begun 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

Category:Pulsars Category:Stars he:פולסר cs:Pulsar da:pulsar de:Pulsar fr:Pulsar it:Pulsar ja:パルサー nl:Pulsar pl:Pulsar sv:Pulsar zh:脉冲星 hu:Pulzár