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Hard X ray Detection and Timing of Accretion Powered Pulsars with BATSE

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Figure

Table 1.1 Accretion-Powered
Table 1.2 Orbital Parameters of Accreting Pulsar Systemsa
Figure 1.2: Spin period versus orbital period for the accreting pulsars with massive com-panions
Figure 2.1: The situated in Compton Gamma Ray Observatory. The 8 BATSE detector modules are on the corners of the spacecraft's main body
+7

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