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- ...nt of a [[star]] or, equivalently, a [[white dwarf]] or a [[magnetar]]<ref>Magnetars have enormous magnetic flux densities on their surfaces due to the small ra ...fields ∼10<sup>11−15</sup> [[gauss (unit)|G]] ('classical' radio pulsars, 'magnetars', X-ray pulsars), whereas old neutron stars have weak fields ≲ 10<sup>9</su ...11 KB (1,522 words) - 16:56, 19 January 2025
- 10 KB (1,331 words) - 23:32, 10 April 2024
- {{Expand section|need expansion on energy release per nucleon reaction in magnetars. It requires an explanation of the arbitrary unit B* that the study has bui ...24 KB (3,407 words) - 15:02, 29 October 2024
- ====Pulsars and magnetars==== ...60 KB (8,880 words) - 18:06, 15 February 2025
- ...|access-date=11 June 2020 }}</ref> Further studies support the notion that magnetars may be closely associated with FRBs.<ref name="SCD-20201226">{{cite news |a ...ay]], which originated from the magnetar [[SGR 1935+2154]], indicates that magnetars may be one source of FRB.<ref name="NASA-20201104" /> ...155 KB (20,398 words) - 06:38, 23 February 2025