Results 171 to 180 of about 3,529,940 (309)
How to build and use special purpose PC clusters in stellar dynamics [PDF]
Rainer Spurzem
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Dynamics of Stellar Collisions
I compare gas-dynamical and stellar-dynamical models of collisions. These two models have distinctly different physics; for example, shocks introduce irreversibility in gas systems, while stellar systems evolve in a completely reversible fashion. Nonetheless, both models yield broadly similar results, suggesting that analogies between gas and stellar ...
openaire +2 more sources
The Escape Velocity Profile of the Milky Way from Gaia DR3
The escape velocity profile of the Milky Way offers a crucial and independent measurement of its underlying mass distribution and dark matter (DM) properties.
Cian Roche +4 more
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Collisional Shaping of Nuclear Star Cluster Density Profiles
A supermassive black hole surrounded by a dense, nuclear star cluster resides at the center of many galaxies. In this dense environment, high-velocity collisions frequently occur between stars.
Sanaea C. Rose, Morgan MacLeod
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We investigate the application of fractional calculus to model stellar dynamics, focusing on resonant relaxation (RR) near a supermassive black hole. Standard theories use the local Fokker–Planck (FP) equation, restricted to Gaussian processes under the ...
Pau Amaro Seoane
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Stellar Evolution and Dynamics in Star Clusters [PDF]
Simon Portegies Zwart +2 more
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The Formation of Stellar Galactic Nuclei through Dissipative Gas Dynamics [PDF]
Kenji Bekki
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Mass Ejection Driven by Sudden Energy Deposition in Stellar Envelopes
A number of stellar astrophysical phenomena, such as tidal novae and planetary engulfment, involve sudden injection of subbinding energy in a thin layer within the star, leading to mass ejection of the stellar envelope.
Nicholas J. Corso, Dong Lai
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Modeling biases from constant stellar mass-to-light ratio assumption in galaxy dynamics and strong lensing [PDF]
Yan Liang +4 more
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