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- W1488703732 abstract "The observed pulsation period of the binary x-ray source 3U 0900--40 can only be explained if the neutron star has a magnetic-field strength Happrox. =10/sup 14/--10/sup 15/ G. (AIP)" @default.
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- W1488703732 date "1975-11-01" @default.
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- W1488703732 title "The long-period x-ray pulsar 3U 0900--40 as a neutron star with an abnormally strong magnetic field" @default.
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