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Criteria for the formation of population III objects in the ultraviolet background radiation
https://ir.soken.ac.jp/records/3291
https://ir.soken.ac.jp/records/32919b8504eb-be1c-47ed-ba70-b9a09762838c
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
j.1365-2966.2001.04669.x (522.6 kB)
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| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2012-12-13 | |||||
| タイトル | ||||||
| タイトル | Criteria for the formation of population III objects in the ultraviolet background radiation | |||||
| タイトル | ||||||
| タイトル | Criteria for the formation of population III objects in the ultraviolet background radiation | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| キーワード | ||||||
| 言語 | en | |||||
| 主題Scheme | Other | |||||
| 主題 | molecular processes,radiative transfer,galaxies, formation,cosmology,theory,diffuse radiation | |||||
| 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 |
KITAYAMA, Tetsu
× KITAYAMA, Tetsu× SUSA, Hajime× UMEMURA, Masayuki× 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 | We explore possibilities of collapse and star formation in Population III objects exposed to the external ultraviolet background (UVB) radiation. Assuming spherical symmetry, we solve self-consistently radiative transfer of photons, non-equilibrium H2 chemistry and gas hydrodynamics. Although the UVB does suppress the formation of low-mass objects, the negative feedback turns out to be weaker than previously suggested. In particular, the cut-off scale of collapse drops significantly below the virial temperature Tvir∼104 K at weak UV intensities (J21≲10−2), owing to both self-shielding of the gas and H2 cooling. Clouds above this cut-off tend to contract highly dynamically, further promoting self-shielding and H2 formation. For plausible radiation intensities and spectra, the collapsing gas can cool efficiently to temperatures well below 104 K before rotationally supported and the final H2 fraction reaches ∼ 10−3. Our results imply that star formation can take place in low-mass objects collapsing in the UVB. The threshold baryon mass for star formation is ∼ 109 M⊙ for clouds collapsing at redshifts z≲3, but drops significantly at higher redshifts. In a conventional cold dark matter universe, the latter coincides roughly with that of the 1σ density fluctuations. Objects near and above this threshold can thus constitute ‘building blocks’ of luminous structures, and we discuss their links to dwarf spheroidal/elliptical galaxies and faint blue objects. These results suggest that the UVB can play a key role in regulating the star formation history of the Universe. |
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| 書誌情報 |
Monthly Notices of the Royal Astronomical Society en : Monthly Notices of the Royal Astronomical Society 巻 326, 号 4, p. 1353-1366, 発行日 2001-10 |
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| 出版者 | ||||||
| 出版者 | Wiley | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 00358711 | |||||
| DOI | ||||||
| 関連タイプ | isIdenticalTo | |||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | https://doi.org/10.1111/j.1365-2966.2001.04669.x | |||||
| 関連名称 | 10.1111/j.1365-2966.2001.04669.x | |||||
| 権利 | ||||||
| 権利情報 | ©2001 The Royal Astronomical Society | |||||
| 関連サイト | ||||||
| 識別子タイプ | URI | |||||
| 関連識別子 | http://www.blackwellpublishing.com/pdf/mnr_caf.pdf | |||||
| 関連名称 | Copyright | |||||
| 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 | VoR | |||||
| 出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
