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Planetary Systems in a Star Cluster II: intermediate-mass black holes and planetary systems

By Francesco Flammini Dotti and others
Most stars form in dense stellar environments. It is speculated that some dense star clusters may host intermediate-mass black holes (IMBHs), which may have formed from runaway collisions between high-mass stars, or from the mergers of less massive black holes. Here, we numerically explore the evolution of populations of planets... Show more
July 23, 2020
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Planetary Systems in a Star Cluster II: intermediate-mass black holes and planetary systems
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