A 4.46 solar-mass black hole is found in a 94-year eccentric orbit with a main-sequence turnoff star in ω Centauri via 23-year astrometric monitoring.
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3 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 3representative citing papers
Reduces elliptic triple outcome model to one free parameter, matches N-body simulations except at low angular momentum, and finds observably eccentric merger fractions of 2.6-4.4% in 10^5-10^7 solar mass clusters.
Bayesian analysis of 163 open clusters finds a universal initial IMF slope of -2.29 with 0.17 scatter and minimal primordial mass segregation, followed by rapid internal mass segregation and later tidal MF flattening.
citing papers explorer
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A Long Period Stellar-Mass Black Hole Binary in $\omega$ Centauri
A 4.46 solar-mass black hole is found in a 94-year eccentric orbit with a main-sequence turnoff star in ω Centauri via 23-year astrometric monitoring.
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Intermediate States in Chaotic Triple Evolution and Applications to Black Hole Merger Statistics
Reduces elliptic triple outcome model to one free parameter, matches N-body simulations except at low angular momentum, and finds observably eccentric merger fractions of 2.6-4.4% in 10^5-10^7 solar mass clusters.
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Evolution of the stellar mass function in open clusters from a universal and unsegregated initial state
Bayesian analysis of 163 open clusters finds a universal initial IMF slope of -2.29 with 0.17 scatter and minimal primordial mass segregation, followed by rapid internal mass segregation and later tidal MF flattening.