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The distribution of stars around the Milky Way's central black hole III. Comparison with simulations 期刊论文
ASTRONOMY & ASTROPHYSICS, 2018, 卷号: 609, 页码: 6
Authors:  Baumgardt, H.;  Amaro-Seoane, P.;  Schodel, R.
Favorite  |  View/Download:1/0  |  Submit date:2018/07/30
methods: numerical  Hertzsprung-Russell and C-M diagrams  stars: kinematics and dynamics  Galaxy: centre  Galaxy: nucleus  
GRAVIDY, a GPU modular, parallel direct-summation N-body integrator: dynamics with softening 期刊论文
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2018, 卷号: 473, 期号: 3, 页码: 3113-3127
Authors:  Maureira-Fredes, Cristian;  Amaro-Seoane, Pau
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methods: numerical  celestial mechanics  stars: kinematics and dynamics  
Revealing the Formation of Stellar-mass Black Hole Binaries: The Need for Deci-Hertz Gravitational-wave Observatories 期刊论文
ASTROPHYSICAL JOURNAL LETTERS, 2017, 卷号: 842, 期号: 1, 页码: 5
Authors:  Chen, Xian;  Amaro-Seoane, Pau
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black hole physics  gravitational waves  methods: analytical  stars: kinematics and dynamics