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   PR # 11047
    Although the globular cluster rotation-powered pulsar is believed to
    be the descendant of LMXBs, the number of LMXB in the globular
    clusters is smaller than what is expected from the number of rotation
    -powered pulsars. This is partly due to the incompleteness of the
    Xray survey of globular cluster LMXB mainly conducted by the Einstein
    Observatory. It is highly important to evaluate the contribution of
    LMXB to the formation ofof rotation-powered pulsars in view of
    investigating the origin of the rotation-powered pulsars.  We thus
    propose to observe the globular clusters with high extinction from
    which it is difficult for Einstein to detect X-ray sources in order
    to completethe survey of LMXBs in the galactic globular clusters.

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