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- W1572358099 abstract "A neutron star in an X-ray binary (XRB) is spun up by mass transfer from its companion to rotation periods of the order of a millisecond. Evidence for this are the existence of ms pulsars, believed to descend from X-ray binaries. Direct evidence of such rotation rates in XRB is the of 2.5 ms rotation in SAX 1808. The rotation energy in a neutron star spinning at 1 ms is 1052 erg, in the range of that required for GRB. The environment also satisfies the baryon loading constraint, since the accretion disk contains only of the order 10−9 M⊙, and the companion star blocks only of the order 1% of the sky as seen from the neutron star." @default.
- W1572358099 created "2016-06-24" @default.
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- W1572358099 date "2000-01-01" @default.
- W1572358099 modified "2023-09-27" @default.
- W1572358099 title "Gamma-ray bursts from rapidly spinning neutron stars" @default.
- W1572358099 doi "https://doi.org/10.1063/1.1361605" @default.
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