#stellar dynamics

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9 papers match

astro-ph.GA2026

Superdiffusion at the Galactic Centre

Pau Amaro Seoane, Kostas Tzanavaris, Reinhard Genzel +14

The paper models the orbital evolution of the S‑star cluster around the Milky Way’s central black hole using a superdiffusive, fractional transport framework that accounts for long…

#galactic centre#stellar dynamics#superdiffusion#fractional transport
astro-ph.GA2026

From S2 to LISA: Astrometric Bounds on Extreme-Mass-Ratio Inspirals and Bursts

Andrea Caputo, Valerie Domcke

The paper uses precise astrometric measurements of the star S2 near the Galactic centre to constrain the number of stellar‑mass black holes and estimate the rates of extreme‑mass‑r…

#stellar dynamics#black hole cusp#extreme mass ratio inspirals#gravitational wave background
astro-ph.GA2026

Stellar rotation of S301 as a macroscopic gyroscope to test general relativity

Pau Amaro Seoane, Xian Chen, Alejandro Torres-Orjuela +16

The paper studies how the rotation of the S301 star near the Galactic Center can act as a macroscopic gyroscope, using its relativistic precession to test general relativity with i…

#stellar dynamics#galactic center#general relativity#gyroscope
astro-ph.GA2026

A Supermassive Black Hole Mass Measurement in NGC 5102 with Schwarzschild Orbit-superposition Modeling

Thomas K. Waters, Kayhan Gultekin, Karl Gebhardt +2

The study determines the mass of the central supermassive black hole in the lenticular galaxy NGC 5102 using stellar-dynamical Schwarzschild orbit-superposition models combined wit…

#supermassive black holes#stellar dynamics#orbit modeling#integral-field spectroscopy
astro-ph.GA2026

Berkeley 32: A Metal-poor and Dynamically Evolved Open Cluster with Evidence of Radial Migration

Deniz Cennet Çınar, D. Bisht, Ing-Guey Jiang +3

The study uses Gaia astrometry and Gaia-ESO spectroscopy to determine the age, metallicity, orbit, binary fraction, and dynamical state of the old, metal-poor open cluster Berkeley…

#open clusters#radial migration#stellar dynamics#chemical abundances
astro-ph.GA2026

Cluster characteristics of Galactic open clusters

K. Neumannová, J. Supíková, N. Faltová +4

The paper estimates total masses, radii, and three‑dimensional shapes for about 7,000 Galactic open clusters using Gaia DR3, 2MASS, and Pan‑STARRS data, and discusses the limitatio…

#open clusters#stellar dynamics#galactic structure#cluster mass estimation