N-body simulations demonstrate that post-capture chaotic planet-planet interactions around pulsars can produce stable low-eccentricity orbits after ejections.
, year = 1993, month = oct, volume =
2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
years
2026 2representative citing papers
Simulations show stars at the edges of stellar streams are more likely to retain unperturbed planetary systems than stars near the stream center.
citing papers explorer
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Formation of stable exoplanetary systems around pulsars by capture: An exercise in computational classical mechanics
N-body simulations demonstrate that post-capture chaotic planet-planet interactions around pulsars can produce stable low-eccentricity orbits after ejections.
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Life is But a Stream: The Distribution of Planetary Systems Along Stellar Streams and their Properties
Simulations show stars at the edges of stellar streams are more likely to retain unperturbed planetary systems than stars near the stream center.