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The neutron star low-mass X-ray binary and intermittent millisecond X-ray pulsar HETE J1900.1–2455 returned to quiescence in late 2015, after a prolonged accretion outburst of ≃10 yr. Using a $\textit{Chandra}$ observation taken ≃180 d into qui
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______109::acb16c76390d4ccbc7979170c6bf4100
https://www.repository.cam.ac.uk/handle/1810/261218
https://www.repository.cam.ac.uk/handle/1810/261218
