PSR J0737−3039 is the first known double pulsar. It consists of two neutron stars emitting electromagnetic waves in the radio wavelength in a relativistic...

due to the emission of gravitational waves, as observed for PSR B1913+16 and PSR J0737−3039. The first radio pulsar was discovered in 1967 by Jocelyn Bell...

stars at apastron (relative to center of mass): 110 km/s Binary pulsar PSR J0737−3039 Square Kilometre Array Tests of general relativity Quadrupole formula...

white dwarf or neutron star. (In at least one case, the double pulsar PSR J0737-3039, the companion neutron star is another pulsar as well.) Binary pulsars...

September 2006, the results of three years of observing a double pulsar, PSR J0737-3039, with the Lovell telescope, as well as with the Parkes and Green Bank...

planets, PSR B1257+12 The first pulsar observed to have been affected by asteroids: PSR J0738−4042 The first double pulsar binary system, PSR J0737−3039 The...

neutron star system where both components are detectable as pulsars, PSR J0737−3039. The discovery of this system allows a total of 5 different tests of...

rotating mass drags the surrounding spacetime with it. Hulse–Taylor pulsar PSR J0737−3039 Bailes, M.; Ord, S. M.; Knight, H. S.; Hotan, A. W. (2003). "Self-Consistency...

percent (by 2005). Multipole radiation Birkhoff's theorem (relativity) PSR J0737−3039 Carroll, Sean M. (2004). Spacetime and Geometry. Pearson/Addison Wesley...

other binary pulsars have been found, in particular the double pulsar PSR J0737−3039, where both stars are pulsars and which was last reported to also be...