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The nature of HI absorption systems at large redshifts
https://ir.soken.ac.jp/records/3643
https://ir.soken.ac.jp/records/3643b1168c3d-701f-4d87-a4ea-9b9083bc06df
| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2013-06-27 | |||||
| タイトル | ||||||
| タイトル | The nature of HI absorption systems at large redshifts | |||||
| タイトル | ||||||
| タイトル | The nature of HI absorption systems at large redshifts | |||||
| 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 | It is proposed that the HI absorption systems in quasars such as the Lyman α forest, Lyman limit systems and damped Lyman α lines are unifiedly understood based upon the expanding clouds confined by the gravity of cold dark matter (CDM). The correlation between these absorption systems and galaxy formation is discussed from the viewpoint of CDM cosmogony. | |||||
| 書誌情報 |
Advances in Space Research en : Advances in Space Research 巻 11, 号 2, p. 245-246, 発行日 1991 |
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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/10.1016/0273-1177(91)90497-8 | |||||
| 関連名称 | 10.1016/0273-1177(91)90497-8 | |||||
| 権利 | ||||||
| 権利情報 | © 1991 Published by Elsevier Ltd | |||||
