The Hulse–Taylor pulsar (known as PSR B1913+16, PSR J1915+1606 or PSR 1913+16) is a binary star system composed of a neutron star and a pulsar which orbit...

decay 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...

pulsars – hence, a "double pulsar" system. The object is similar to PSR B1913+16, which was discovered in 1974 by Jocelyn Bell, Taylor and Hulse, and...

FCRAO labs contributed to the discovery of the binary pulsar system PSR B1913+16 by Joseph Taylor and Russell Hulse, for which they received the 1993...

measured with extraordinary accuracy by radio telescopes. The binary pulsar PSR B1913+16 (or the "Hulse-Taylor binary pulsar") was first discovered in 1974 at...

Russell Hulse discovered for the first time a pulsar in a binary system, PSR B1913+16. This pulsar orbits another neutron star with an orbital period of just...

and angular momentum gradually, as illustrated by the binary pulsar PSR B1913+16. For binary black holes, the numerical solution of the two-body problem...

important class of exact solutions modelling gravitational radiation PSR B1913+16, the first binary pulsar discovered and the first experimental evidence...

Joseph Taylor and Russell Hulse discovered the first binary pulsar, PSR B1913+16, which consists of two neutron stars (one seen as a pulsar) orbiting...

using general relativity. For example, the Hulse–Taylor binary pulsar PSR B1913+16 (a pair of neutron stars in which one is detected as a pulsar) has an...

1970s through observation of a pair of closely orbiting neutron stars, PSR B1913+16. The explanation for the decay in their orbital period was that they...

Mysterious World (1980), and given the more recent discovery of pulsar PSR B1913+16, he said: "How romantic, if even now, we can hear the dying voice of...

deduced in 1974 through the motion of the double neutron star system PSR B1913+16, in which one of the stars is a pulsar that emits electro-magnetic pulses...

PSR J0952–0607 with a reported mass of 2.35+0.17 −0.17 M☉. PSR J0740+6620 is estimated to measure 12.39+1.30 −0.98 km (7.70+0.81 −0.61 mi). PSR B1913+16...

binary pulsar PSR B1913+16, an accomplishment for which they later received the Nobel Prize in Physics. In 1982, the first millisecond pulsar, PSR B1937+21...

J. H. (2010). "Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16". Astrophysical Journal. 722 (2): 1030–1034. arXiv:1011.0718. Bibcode:2010ApJ...

Hulse and Taylor discovered the first pulsar in a binary system, named PSR B1913+16 after its position in the sky, during a survey for pulsars at the Arecibo...

Joel Weisberg show that the rate of energy loss from the binary pulsar PSR B1913+16 agrees with that predicted by the general relativistic quadrupole formula...

type, 1974 – Russell Hulse and Joseph Taylor discover the binary pulsar PSR B1913+16. 1977 – Kip Thorne and Anna Żytkow present a detailed analysis of Thorne–Żytkow...

POLYGON experiment POVM PQS (chemical) PS210 experiment PSR B1828-10 PSR B1913+16 PSR J0737-3039 PSR J1614–2230 PUREX PVLAS PVT (physics) PWscf PYTHIA Padma...

long-period variable star (not a nova) in Cygnus The Hulse–Taylor binary is PSR B1913+16 (a binary pulsar) in Aquila. Named after Russell Alan Hulse and Joseph...

(October 20, 2010). "Timing Measurements of the Relativistic Binary Pulsar PSR B1913+16". The Astrophysical Journal. 722 (2): 1030–1034. arXiv:1011.0718. Bibcode:2010ApJ...

solar masses, similar to the mass of the most massive double neutron star, B1913+16. Timing analysis of 13 radio pulsars discovered by Einstein@Home were published...

Weisberg, Joel M.; Taylor, Joseph H. (2003), "The Relativistic Binary Pulsar B1913+16"", in Bailes, M.; Nice, D. J.; Thorsett, S. E. (eds.), Proceedings of "Radio...