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A non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a carbon atmosphere
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Our timing analysis did not reveal any pulsations with a pulsed fraction above ~8% down to 0.2 ms. This finding further supports the hypothesis that the emitting surface area is the entire neutron star surface.
No X-ray pulsations have been detected from the compact object in HESS J1731-347
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Drawn on by · none recordedA non-pulsating neutron star in the supernova remnant HESS J1731-347/G353.6-0.7 with a ca…
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- Link
- https://www.aanda.org/articles/aa/full_html/2013/08/aa21740-13/aa21740-13.html
- Archived copy
- https://web.archive.org/web/20260608082132/https://www.aanda.org/articles/aa/full_html/2013/08/aa21740-13/aa21740-13.html
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- Facts checked
- Nov 9, 2026
History 2
- Nov 9, 2026FactsFacts fetcher · Facts looked up
- Aug 5, 2026Entered the graphEntered the graph; no copy stored