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Formation of intermediate-mass black holes in circumnuclear regions of galaxies
https://ir.soken.ac.jp/records/3295
https://ir.soken.ac.jp/records/3295723d36e6-87a6-4221-9cd7-703a19fa2362
名前 / ファイル | ライセンス | アクション |
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Item type | 学術雑誌論文 / Journal Article(1) | |||||
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公開日 | 2012-12-13 | |||||
タイトル | ||||||
タイトル | Formation of intermediate-mass black holes in circumnuclear regions of galaxies | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Formation of intermediate-mass black holes in circumnuclear regions of galaxies | |||||
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 | |||||
著者 |
TANIGUCHI, Yoshiaki
× TANIGUCHI, Yoshiaki× SHIOYA, Yasuhiro× TSURU, Takeshi G× 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 | Recent high-resolution X-ray imaging studies have discovered possible candidates of intermediate-mass black holes with masses of $M_\bullet \sim 10^{2-4} \MO$ in circumnuclear regions of many (disk) galaxies. It is known that a large number of massive stars are formed in a circumnuclear giant H {\sc ii} region. Therefore, we propose that continual merger of compact remnants left from these massive stars is responsible for the formation of such an intermediate-mass black hole within a timescale of $\sim 10^9$ years. A necessary condition is that several hundreds of massive stars are formed in a compact region with a radius of a few pc. | |||||
書誌情報 |
Publications of the Astronomical Society of Japan en : Publications of the Astronomical Society of Japan 巻 52, 号 3, p. 533-537, 発行日 2000-02 |
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ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 00046264 | |||||
権利 | ||||||
権利情報 | © Y. Taniguchi et al. | |||||
関連サイト | ||||||
識別子タイプ | URI | |||||
関連識別子 | http://arxiv.org/abs/astro-ph/0002389 | |||||
関連名称 | arXiv:astro-ph/0002389 | |||||
フォーマット | ||||||
内容記述タイプ | Other | |||||
内容記述 | application/pdf | |||||
著者版フラグ | ||||||
出版タイプ | AM | |||||
出版タイプResource | http://purl.org/coar/version/c_ab4af688f83e57aa |