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Evolution of disk galaxies regulated by supernova remnants
https://ir.soken.ac.jp/records/3517
https://ir.soken.ac.jp/records/35174a91c2ee-ee09-411e-9d07-32e1a98e7cc8
| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2013-04-25 | |||||
| タイトル | ||||||
| タイトル | Evolution of disk galaxies regulated by supernova remnants | |||||
| タイトル | ||||||
| タイトル | Evolution of disk galaxies regulated by supernova remnants | |||||
| 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 |
TANAKA, Yutaka D.
× TANAKA, Yutaka D.× IKEUCHI, Satoru× HABE, Asao |
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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 | Assuming that a disk galaxy is composed of an ambient pervasive gas, small clouds, molecular clouds and stars, its evolution is studied through examining the interchange processes among them. Main results obtained are: (1) The star formation rate is directed by the formation process of molecular clouds. (2) Depending upon the parameters there may be three or four types of evolution of disk galaxies: the no star formation case, the active in the past and inactive at present star formation case, the burst-like star formation case and the very active in star formation case. | |||||
| 書誌情報 |
Astrophysical Journal Letters en : Astrophysical Journal Letters 巻 119, 号 1, p. 207-210, 発行日 1986-01 |
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| 出版者 | ||||||
| 出版者 | SpringerLink | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 20418205 | |||||
| DOI | ||||||
| 識別子タイプ | DOI | |||||
| 関連識別子 | https://doi.org/10.1007/BF00648848 | |||||
| 関連名称 | 10.1007/BF00648848 | |||||
| 権利 | ||||||
| 権利情報 | SpringerLink(The original publication is available at www.springerlink.com) | |||||
