Observations of Accreting Pulsars
We discuss recent observations of accreting binary pulsars with the all-sky BATSE instrument on the Compton Gamma Ray Observatory. BATSE has detected and studied nearly half of the known accreting pulsar systems. Continuous timing studies over a two-year period have yielded accurate orbital parameters for 9 of these systems, as well as new insights into long-term accretion torque histories.
Additional Information© 1994 American Institute of Physics. We acknowledge the important contributions of the entire BATSE team at NASA/Marshall Space Flight Center to this work. We recognize in particular the individual contributions of M. Briggs, J. Chiu, G. J. Fishman, L. Gibby, J. M. Grunsfeld, B. A. Harmon, T. Koh, C. A. Meegan, W. S. Paciesas, G. N. Pendleton, B. C. Rubin, M. T. Stollberg, C. A. Wilson, and N. S. Zhang. This work is funded in part by NASA grants NAGW-1919, NAG 5-1458, NGT-51184 and a Lee A. DuBridge fellowship to L.B. funded by the Weingart Foundation.
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