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Feedback of AGN turn-on in galaxies
https://ir.soken.ac.jp/records/3642
https://ir.soken.ac.jp/records/36427639575d-5eac-48ec-b4ec-f0a860b01052
Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2013-06-27 | |||||
タイトル | ||||||
タイトル | Feedback of AGN turn-on in galaxies | |||||
タイトル | ||||||
タイトル | Feedback of AGN turn-on in galaxies | |||||
言語 | en | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | journal article | |||||
アクセス権 | ||||||
アクセス権 | metadata only access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_14cb | |||||
著者 |
IKEUCHI, Satoru
× IKEUCHI, Satoru |
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著者別名 |
池内, 了
× 池内, 了 |
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抄録 | ||||||
内容記述タイプ | Abstract | |||||
内容記述 | Many lines of evidence for the presence of massive black holes in AGN are presented here. The nuclei of normal galaxies also show similar activity to AGN, though their energy outputs are smaller by several orders of magnitude. This similarity suggests that massive black holes exist in all normal galaxies but the activity is weak due to some unknown mechanism. Here, I review recent work that revives an old accretion disk model which represents four types of activity, depending upon the mass of a central black hole and the gas accretion rate. These four types of solutions may correspond to the levels of activity in AGN and normal galaxies. | |||||
書誌情報 |
Advances in Space Research en : Advances in Space Research 巻 23, 号 5-6, p. 856-870, 発行日 1999 |
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出版者 | ||||||
出版者 | Elsevier | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 02731177 | |||||
DOI | ||||||
識別子タイプ | DOI | |||||
関連識別子 | http://doi.org/10.1016/S0273-1177(99)00214-8 | |||||
関連名称 | 10.1016/S0273-1177(99)00214-8 | |||||
権利 | ||||||
権利情報 | © 1999 Published by Elsevier Ltd. |