PSR J1930–1852
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PSR J1930–1852 is a binary pulsar system, composed of a pulsar and a neutron star and orbiting around their common center of mass. Located Template:Convert away from Earth in the constellation Sagittarius, it is the most distantly-separated double neutron star system known.[1][2][3]
See also
- Hulse–Taylor binary, first pulsar in a binary system discovered
- PSR J0737−3039, first double pulsar binary system discovered
- PSR J1946+2052, double neutron star system with the shortest known orbital period