The discovery of the largest timing irregularity yet observed in a pulsar is the first confirmation that binary pulsars (pulsars orbiting with a companion white dwarf or neutron star) exhibit the phenomenon known as a glitch. Composite image of the X-ray pulsar SXP 1062 surrounded by the supernova remnant. The false-color image combines X-ray (blue) and optical data (oxygen – green, hydrogen – red). Image credit: ESA / XMM-Newton / L....
