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Evolution of Supernova Remnants. 1. Interacting Supernova Remnants
https://ir.soken.ac.jp/records/3313
https://ir.soken.ac.jp/records/3313451855ca-28b2-46c4-82b6-24c22d81ee27
| Item type | 学術雑誌論文 / Journal Article(1) | |||||
|---|---|---|---|---|---|---|
| 公開日 | 2013-01-09 | |||||
| タイトル | ||||||
| タイトル | Evolution of Supernova Remnants. 1. Interacting Supernova Remnants | |||||
| タイトル | ||||||
| タイトル | Evolution of Supernova Remnants. 1. Interacting Supernova Remnants | |||||
| 言語 | en | |||||
| 言語 | ||||||
| 言語 | eng | |||||
| キーワード | ||||||
| 言語 | en | |||||
| 主題Scheme | Other | |||||
| 主題 | Interstellar matter,Shock waves,Supernova remnants,X-rays | |||||
| 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 | The evolution and structure of two interacting supernova remnants (SNRS) are calculated by use of a timedependent two-dimensional hydro- dynamic code. The interactions of two SNRs are simulated in such a Way that at a time t。 after the first supernova explosion, the second Supernova explosion occurs at the distance D and two SNRs encounter. Two cases are investigated; the second explosion occurs outside or in- Side the expanding she11 0f the first SNR.I n the first case, the final Structures of two interacting SNRs are typica11y classified into three types:(1) two SNRs merge into a single-1ike SNR,(2) two SNRs merge but show a peanut-shape structure, and (3) two SNRs do not merge.1n the second case, they reduce to two types:(1) Two SNRs evolve as an isolated SNR with twice the explosion energy, and (2) in the she11 of the first SNR a bump is formed due to the shock impact by the second ex- Plosion. The critical distances for the above structural changes are examined, as we11 as the changes ot the expansion law trom an isolated SNR. With these results some discussions are given on the formation of an SNR tunnel system and the possibility of gas ejection from a galaxy. Based upon this view' of interacting SNRS, a preliminary model for the solar neighborhood and loop l is presented. |
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| 書誌情報 |
Publications of the Astronomical Society of Japan en : Publications of the Astronomical Society of Japan 巻 30, p. 563-580, 発行日 1978-10 |
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| 出版者 | ||||||
| 出版者 | The Astronomical Society of Japan | |||||
| ISSN | ||||||
| 収録物識別子タイプ | ISSN | |||||
| 収録物識別子 | 00046264 | |||||
| 権利 | ||||||
| 権利情報 | © The Astronomical Society of Japan | |||||
| 関連サイト | ||||||
| 識別子タイプ | URI | |||||
| 関連識別子 | http://pasj.asj.or.jp/info/subscription.html | |||||
| 関連名称 | Copyright | |||||
| 関連サイト | ||||||
| 識別子タイプ | URI | |||||
| 関連識別子 | http://adsabs.harvard.edu/full/1978PASJ...30..563I%7CCited | |||||
| 関連名称 | The Astronomical Society of Japan | |||||
| 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 | |||||
