A non-pulsating neutron star in the supernova remnant HESS J1731−347/G353.6−0.7 with a carbon atmosphere

@article{Klochkov2013ANN,
  title={A non-pulsating neutron star in the supernova remnant HESS J1731−347/G353.6−0.7 with a carbon atmosphere},
  author={D. Klochkov and G. Puehlhofer and V. Suleimanov and S. Simon and K. Werner and A. Santangelo},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={556}
}
Context. The CCO (central compact object) candidate in the center of the supernova remnant shell HESS J1731−347 / G353.6−0.7 shows no pulsations and exhibits a blackbody-like X-ray spectrum. If the absence of pulsations is interpreted as eviden ce for the emitting surface area being the entire neutron star surface , the assumption of the measured flux being due to a blackbody e mission translates into a source distance that is inconsistent with current estimates of the remnant’s distance. Aims… Expand

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XMM-Newton observations of the non-thermal supernova remnant HESS J1731-347 (G353.6-0.7)
X-ray spectral analysis of the neutron star in SNR 1E 0102.2-7219
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