Triaxial dynamical modelling of the Galactic centre recovers the known mass of Sgr A* and shows the nuclear structures are mildly triaxial with radially varying orbit populations dominated by hot/warm orbits inside a few parsecs and cold orbits farther out.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2representative citing papers
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
citing papers explorer
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A spectroscopic map of the Galactic centre: Integrated light and dynamical modelling
Triaxial dynamical modelling of the Galactic centre recovers the known mass of Sgr A* and shows the nuclear structures are mildly triaxial with radially varying orbit populations dominated by hot/warm orbits inside a few parsecs and cold orbits farther out.
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Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.