Abstract
This is the third and last of a series of papers dedicated to the effect of triple encounters with the formation of a binary and escape of the third body on the evolution of stellar systems. Previously obtained results are applied to several astronomical models of triplets formed by sun-like stars, white dwarfs and neutron stars.
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Chandra, N., Bhatnagar, K. Applications of Two-Parameter Families of Triple Encountersto Stellar Systems (III). Astrophysics and Space Science 271, 423–431 (2000). https://doi.org/10.1023/A:1002445503238
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DOI: https://doi.org/10.1023/A:1002445503238