轻弹
发表于 2025-3-30 09:13:48
Generalized Flows Around Neutron Starse NSs. We showcase some of our findings from Monte Carlo and Smoothed Particle Hydrodynamic simulations which further strengthens the points raised in Sect. 4. In summary, we remark on the possibility of future works using TCAF for both weakly magnetic and magnetic Neutron Stars.
类人猿
发表于 2025-3-30 15:45:30
Formation of Two Component Flows by Numerical Simulations Around Black Holesway from the equatorial plane behaves like a transonic flow with standing and oscillating shocks. Finally, we observed that, our solution is consistent with the Chakrabarti-Titarchuk two-component advective flow configuration as the flow approaches to a black hole.
CHASE
发表于 2025-3-30 19:04:52
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参考书目
发表于 2025-3-31 00:37:33
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法律的瑕疵
发表于 2025-3-31 02:16:23
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Pillory
发表于 2025-3-31 05:39:38
Radiation Characteristics of Two-Component Accretion Flow Paradigm Around Black Holesermassive black holes. Also, two-component advective solutions can be used to understand the triggering of outburst events in compact X-ray sources due to sudden surge of viscosity or mass accretion at the outer boundary.
nuclear-tests
发表于 2025-3-31 13:13:33
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可卡
发表于 2025-3-31 14:44:57
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arthrodesis
发表于 2025-3-31 20:05:30
Spinning Black Holes, Spinning Flows and Spinorsed to be rotating, however be the magnitude of angular speed. The generalized astrophysical black hole is the rotating one (the Kerr black hole) which often accretes matter from its surrounding (e.g. from its binary companion) forming an accretion disk (namely X-ray binary). This accretion disk is t
chisel
发表于 2025-3-31 23:06:35
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