The double pulsar system J0737-3039

@article{Lyne2006TheDP,
  title={The double pulsar system J0737-3039},
  author={Andrew G. Lyne},
  journal={New Astronomy Reviews},
  year={2006},
  volume={54},
  pages={135-139}
}
  • A. Lyne
  • Published 1 March 2010
  • Physics
  • New Astronomy Reviews

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References

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The Double Pulsar System J0737–3039: Modulation of the Radio Emission from B by Radiation from A
We have analyzed single pulses from PSR J0737-3039B, the 2.8 s pulsar in the recently discovered double pulsar system, using data taken with the Green Bank Telescope at 820 and 1400 MHz. We report
A Double-Pulsar System: A Rare Laboratory for Relativistic Gravity and Plasma Physics
TLDR
The detection of the 2.8-second pulsar J0737–3039B as the companion to the 23-millisecond pulsars in a highly relativistic double neutron star system, allowing unprecedented tests of fundamental gravitational physics.
Studies of the Relativistic Binary Pulsar PSR B1534+12. I. Timing Analysis
We have continued our long-term study of the double neutron star binary pulsar PSR B1534+12, using new instrumentation to make very high precision measurements at the Arecibo Observatory. We have
The Double Pulsar System J0737-3039: Modulation of A by B at Eclipse
We have investigated the eclipse of the 23 ms pulsar, PSR J0737-3039A, by its 2.8 s companion PSR J0737-3039B in the recently discovered double pulsar system using data taken with the Green Bank
The mean pulse profile of PSR J0737-3039A
General relativity predicts that the spin axes of the pulsars in the double-pulsar system PSR J0737-3039A/B will precess rapidly, in general leading to a change in the observed pulse profiles. We
An increased estimate of the merger rate of double neutron stars from observations of a highly relativistic system
TLDR
This work reports the discovery of a 22-ms pulsar, PSR J0737–3039, which is a member of a highly relativistic double-neutron-star binary with an orbital period of 2.4 hours, which implies an order-of-magnitude increase in the predicted merger rate for double- NEUTron- star systems in the authors' Galaxy (and in the rest of the Universe).
Determination of the Geometry of the PSR B1913+16 System by Geodetic Precession
New observations of the binary pulsar B1913+16 are presented. Since 1978 the leading component of the pulse profile has weakened dramatically by about 40%. For the first time, a decrease in component
Further experimental tests of relativistic gravity using the binary pulsar PSR 1913+16
Fourteen-year observations of the binary pulsar PSR 1913 + 16 provided data consistent with a straightforward model allowing for the motion of the earth, special and general relativistic effects
THE COSMIC COALESCENCE RATES FOR DOUBLE NEUTRON STAR BINARIES
We report on the newly increased event rates due to the recent discovery of the highly relativistic binary pulsar J07373039. Using a rigorous statistical method, we present the calculations reported
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