A First XMM-Newton Look at the Relativistic Double Pulsar PSR J0737-3039

@article{Pellizzoni2004AFX,
  title={A First XMM-Newton Look at the Relativistic Double Pulsar PSR J0737-3039},
  author={Alberto Pellizzoni and Andrea De Luca and Sandro Mereghetti and Andrea Tiengo and Fabio Mattana and Patrizia A. Caraveo and Marco Tavani and Giovanni Fabrizio Bignami},
  journal={The Astrophysical Journal},
  year={2004},
  volume={612}
}
We present the results of a 50 ks long X-ray observation of the relativistic double pulsar system PSR J0737-3039 obtained with the XMM-Newton satellite in 2004 March. The source has a soft spectrum (with a power-law photon index of 3.5 ) and a 0.2-10 keV luminosity of ~3 × 1030 ergs s-1 (assuming a distance of 500 pc), consistent with the values derived from a previous Chandra observation. No flux variations have been detected, implying the absence of large orbital modulations. The high time… 
XMM-Newton Observation of the Double Pulsar System J0737?3039
We report on a 50 ks XMM-Newton observation of the double pulsar system J0737-3039 performed in 2004 April. We present results of the spectral analysis of these data combined with the much shorter
PSR J0737-3039 : INTERACTING PULSARS IN X-RAYS
We present the results of a ~230 ks long X-ray observation of the relativistic double-pulsar system PSR J0737–3039 obtained with the XMM-Newton satellite in 2006 October. We confirm the detection in
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We present a long-term spectral monitoring of the unique Double Pulsar binary PSR J0737-3039 corresponding to two "Large Programs" performed by XMM-Newton in 2006 and 2011. Spectral variability of
LONG-TERM STUDY OF THE DOUBLE PULSAR J0737–3039 WITH XMM-NEWTON: PULSAR TIMING
The relativistic double neutron star binary PSR J0737-3039 shows clear evidence of orbital phase-dependent wind-companion interaction, both in radio and X-rays. In this paper we present the results
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The relativistic double neutron star binary PSR J0737–3039 is a truly unique system offering the diagnostics of two interacting radio pulsars in a short orbital period system. Clear evidences of
The very soft X-ray spectrum of the double pulsar system J0737-3039
We present the results of an 80 ks Chandra ACIS-S observation of the double pulsar system J0737-3039. Furthermore, we report on spectral, spatial and timing analysis of the combined X-ray
Radio Emission from the Double-Pulsar System J0737–3039 Revisited
The double pulsar J0737-3039 is the only known system in which the relativistic wind emitted by a radio pulsar demonstrably interacts with the magnetosphere of another one. We report radio
Pulsed X-Ray Emission from Pulsar A in the Double Pulsar System J0737–3039
The double pulsar system J0737-3039 is not only a test bed for general relativity and theories of gravity, but also provides a unique laboratory for probing the relativistic winds of neutron stars.
Observations of the Double Pulsar PSR J0737-3039A/B
The double pulsar J0737-3039A/B consists of a recycled 22-millisecond pulsar and a young 2.7-second pulsar in a highly relativistic 2.4-hour orbit. This system provides an unprecedented laboratory
Hubble Space Telescope detection of the double pulsar system J0737−3039 in the far-ultraviolet
We report on detection of the double pulsar system J0737–3039 in the far-UV with the Advanced Camera for Surveys/Solar-blind Channel detector aboard Hubble Space Telescope. We measured the energy
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