Bibliographic Information
- Other Title
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- Structure Around the Inner Edge of Geom
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Abstract
type:Article
In geometrically thin, nearly Keplerian disks, there is an inner edge inside which the gas falls toward the black hole by dynamical instability due to a relativistic effect. The disk structure around this edge is examined in detail when the geometry is Schwarzschildian and the vertically averaged kinematic viscosity is constant. A steady disk model is found in which the disk structure changes continuously at the edge from a nearly Keplerian structure to a thin non-Keplerian structure of the infalling gas. The structure of this transition region is demonstrated.
Journal
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- Publications of the Astronomical Society of Japan
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Publications of the Astronomical Society of Japan 34 51-63, 1982
Astronomical Society of Japan
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Details 詳細情報について
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- CRID
- 1050564287756414848
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- NII Article ID
- 120002108199
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- NII Book ID
- AA00795296
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- ISSN
- 00046264
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- NDL BIB ID
- 2441308
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- Text Lang
- en
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- Article Type
- journal article
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- Data Source
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- IRDB
- NDL
- CiNii Articles