Results 311 to 320 of about 225,051 (342)
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2005
The properties of instabilities occurring in thick disks are reviewed. Their origin and mechanism is discussed and a summary of the influence of various model parameters and stabilising effects is given.
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The properties of instabilities occurring in thick disks are reviewed. Their origin and mechanism is discussed and a summary of the influence of various model parameters and stabilising effects is given.
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Meridional flow in thick accretion disks
Astrophysics and Space Science, 1989We have studied the effect of the flow in the accretion disk. The specific angular momentum of the disk is assumed to be constant and the polytropic relation is used. We have solved the structure of the disk and the flow patterns of the irrotational perfect fluid.
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The merger that led to the formation of the Milky Way’s inner stellar halo and thick disk
Nature, 2018Amina Helmi +2 more
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Hierarchical 3D electrodes for electrochemical energy storage
Nature Reviews Materials, 2018Hongtao Sun, Jian Zhu, Lele Peng
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Foundations of Black Hole Accretion Disk Theory
Living Reviews in Relativity, 2013P Chris Fragile
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