In this paper, the second of a series, we study the stellar dynamical and evolutionary processes leading to the formation of compact binaries containing neutron stars (NSs) in dense globular clusters. For this study, 70 dense clusters were simulated independently, with a total stellar mass 2 10 7 M , exceeding the total mass of all dense globular clusters in our Galaxy.
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Ivanova et al. (2008) studied this question.
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