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Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:3405-3411
High mass accretion rate onto strongly magnetised neutron stars results in the appearance of accretion columns supported by the radiation pressure and confined by the strong magnetic field of a star. At mass accretion rates above $\sim 10^{19}\,{\rm
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9ec4984544bb0f2fd4ef5d97b7c9bd07
https://doi.org/10.1093/mnras/stad1118
https://doi.org/10.1093/mnras/stad1118
