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2 results

  • The maximum spin of Millisecond Pulsar and the gravitational wave

  • C. M. Zhang
  • Journal:
    Proceedings of the International Astronomical Union / Volume 11 / Issue A29B / August 2015
    Published online by Cambridge University Press:
    27 October 2016, pp. 370-371
    Print publication:
    August 2015
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  • The gravitational wave radiation will release the energy momentum, which will dissipate the rotation of neutron star while in the accretion process. If the deformation of star is known, then we can estimate the maximum spin frequency of pulsar, based on which we can interpret why the spin periods of all millisecond pulsars cannot be less than one millisecond.

  • Minimum accretion rate for millisecond pulsar formation in binary system

  • Yuanyue Pan, Chengmin Zhang, Na Wang
  • Journal:
    Proceedings of the International Astronomical Union / Volume 8 / Issue S290 / August 2012
    Published online by Cambridge University Press:
    21 February 2013, pp. 291-292
    Print publication:
    August 2012
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  • 186 binary pulsars are shown in the magnetic field versus spin period (B-P) diagram, and their relations to the millisecond pulsars can be clearly seen. We declaim a minimum accretion rate for the millisecond pulsar formation both from the observation and theory. If the accretion rate is lower than the minimum accretion rate, the pulsar in binary system will not become a millisecond pulsar after the evolution.