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357472A0
357472A0
http://dx.doi.org/10.1038/357472A0
Millisecond pulsars with extremely strong magnetic fields as a cosmological source of γ-ray bursts
P356
Q59092798-065E9D7F-F748-4168-8DAD-EA99CD04B052
P356
357472A0
http://dx.doi.org/10.1038/357472A0