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• W2022044745 endingPage "563" @default.
• W2022044745 startingPage "561" @default.
• W2022044745 abstract "Probing Pulsar Rotation Pulsars are strongly magnetized, rapidly rotating neutron stars. Those with periods of the order of milliseconds obtain their fast spin by accreting mass from a companion star in a binary system. Tauris (p. 561 ) combined numerical stellar evolution calculations with a model of how accretion torques act on a neutron star. During the late accretion phase of millisecond pulsars, the termination stage of mass transfer results in a loss of more than 50% of their rotational energy. This effect may explain the observed pulsar spin distributions." @default.
• W2022044745 created "2016-06-24" @default.
• W2022044745 creator A5000032138 @default.
• W2022044745 date "2012-02-03" @default.
• W2022044745 modified "2023-10-17" @default.
• W2022044745 title "Spin-Down of Radio Millisecond Pulsars at Genesis" @default.
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• W2022044745 doi "https://doi.org/10.1126/science.1216355" @default.
• W2022044745 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/22301314" @default.
• W2022044745 hasPublicationYear "2012" @default.
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