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Bibliographic Record
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- Material Type
- 文書・図像類
- Author/Editor
- 和田, 桂一
- Author Heading
- Publication, Distribution, etc.
- Alternative Title
- Structures around aupermassive black holes and their evolution: feedback and feeding
- Text Language Code
- jpn
- Target Audience
- 一般
- Note (General)
- 2011-2013年度科学研究費助成事業（基盤研究（C））研究成果報告書 課題番号：23540267 研究代表者：和田桂一（鹿児島大学・理工学研究科・教授）銀河中心の巨大ブラックホール近傍10パーセクから降着円盤領域にかけての空間スケールで6桁にわたる領域の構造を解明すべく理論的研究を行った。高精度の3次元輻射流体計算等により、降着円盤からの強い輻射による加熱と輻射圧によって、星間ガスのアウトフローが発生することを明らかにした。このアウトフローは、巨大ブラックホールの活動性の起源である「質量降着」（ガスの内向きの流れ）を妨げない。アウトフローは非定常かつ非一様であり、その進化の結果、「遮蔽トーラス」が自然に形成されることを示した。降着円盤の領域では輝線で駆動された高速のアウトフローが形成され、幅広い吸収線を持つクェーサーの種族の起源に迫った。We have theoretically investigated structures and dynamics of the ISM around super massive black holes in galaxies. Using three-dimensional radiation-hydrodynamics simulations, we confirmed that non-steady and non-uniform outflows are generated due to the radiation pressure and heating. This outflow does not prevent from accreting materials toward the galactic center. We also found that a part of failed outflows naturally form an obscuring torus, which has been postulated to explain observed properties of AGNs. The radiation-driven outflows are ubiquitous over a large dynamic range, for example, we found that strong line-driven winds are formed from the accretion disk, and this consistently explains broad-absorption line quasars.