ORBITAL VARIATION OF THE X-RAY EMISSION FROM THE DOUBLE NEUTRON STAR BINARY J1537+1155

@article{Durant2011ORBITALVO,
  title={ORBITAL VARIATION OF THE X-RAY EMISSION FROM THE DOUBLE NEUTRON STAR BINARY J1537+1155},
  author={M. Durant and O. Kargaltsev and I. Volkov and G. Pavlov},
  journal={The Astrophysical Journal},
  year={2011},
  volume={741},
  pages={65}
}
We observed the double neutron star binary (DNSB) containing PSR J1537+1155 (also known as B1534+12) with the Chandra X-Ray Observatory. This is one of the two DNSBs detected in X-rays and the only one where a hint of variability with orbital phase was found (in the previous Chandra observation). Our follow-up observation supports the earlier result: the distribution of photon arrival times with orbital phase again shows a deficit around apastron. The significance of the deficit in the combined… Expand

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References

SHOWING 1-10 OF 25 REFERENCES
X-ray emission from the double pulsar system J0737-3039
The very soft X-ray spectrum of the double pulsar system J0737-3039
DETECTION OF X-RAY EMISSION FROM THE VERY OLD PULSAR J0108-1431
X-Ray Emission from the Planet Pulsar B1257+12
The double pulsar: evolutionary constraints from the system geometry
On the nature of eclipses in binary pulsar J0737–3039
Tests of General Relativity from Timing the Double Pulsar
PSR J0737-3039 : INTERACTING PULSARS IN X-RAYS
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