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Interaction of intergalactic-gas flow with a rigid-body, spheroidal galaxy
https://ir.soken.ac.jp/records/3645
https://ir.soken.ac.jp/records/364556b68e45-dbf6-4c89-8be5-b9d018f11752
| 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 | Interaction of intergalactic-gas flow with a rigid-body, spheroidal galaxy | |||||||||
| タイトル | ||||||||||
| タイトル | Interaction of intergalactic-gas flow with a rigid-body, spheroidal galaxy | |||||||||
| 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
× TOMISAKA, Kohji
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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 | The interaction of intergalactic-gas flow, which is assumed to be an incompressible fluid, with a rigid-body, spheroidal galaxy is examined analytically. The gas-flow patterns, the distributions of pressure at the surface of galaxy and some other quantities are calculated for the cases with and without viscosity. By use of results, we discuss the formation of HI ridges, trailing clouds and gas streams accompanying with galaxies, and the bending (or warping) of intersteller gas observed in spiral galaxies are analyzed. Some discussion on the Magellanic Stream is given. | |||||||||
| 書誌情報 |
Astrophysics and Space Science en : Astrophysics and Space Science 巻 80, 号 2, p. 483-500, 発行日 1981-12 |
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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 | 0004640X | |||||||||
| DOI | ||||||||||
| 識別子タイプ | DOI | |||||||||
| 関連識別子 | http://doi.org/10.1007/BF00652947 | |||||||||
| 関連名称 | 10.1007/BF00652947 | |||||||||
| 権利 | ||||||||||
| 権利情報 | SpringerLink(The original publication is available at www.springerlink.com) | |||||||||
