Abstract
The tidal breakup of a neutron star near a black hole is examined. A simple model for the interaction is calculated, and the results show that the amount of neutron-star material ejected into the interstellar medium may be significant. Using reasonable stellar statistics, the estimated quantity of ejected material is found to be roughly comparable to abundance of r-process material.
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CITATION STYLE
APA
Lattimer, J. M., & Schramm, D. N. (1974). Black-hole-neutron-star collisions. The Astrophysical Journal, 192, L145. https://doi.org/10.1086/181612
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