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The Cycling of Matter between Stars, the Interstellar Medium, and the Intergalactic Medium
https://jaxa.repo.nii.ac.jp/records/3014
https://jaxa.repo.nii.ac.jp/records/3014c341ae86-cc9c-4c0f-9975-d3e5674302e0
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
AA1730027037.pdf (10.8 MB)
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| Item type | 会議発表論文 / Conference Paper(1) | |||||||
|---|---|---|---|---|---|---|---|---|
| 公開日 | 2018-05-01 | |||||||
| タイトル | ||||||||
| タイトル | The Cycling of Matter between Stars, the Interstellar Medium, and the Intergalactic Medium | |||||||
| 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_5794 | |||||||
| 資源タイプ | conference paper | |||||||
| 著者 |
Tielens, A. G. G. M.
× Tielens, A. G. G. M.
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| 著者所属（英） | ||||||||
| en | ||||||||
| Leiden University | ||||||||
| 出版者 | ||||||||
| 出版者 | 宇宙航空研究開発機構(JAXA) | |||||||
| 出版者（英） | ||||||||
| 出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||||
| 書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe 巻 JAXA-SP-17-010E, p. 163-171, 発行日 2018-03-09 |
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| 会議概要（会議名, 開催地, 会期, 主催者等）（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan | |||||||
| 抄録（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | The evolution of the interstellar medium is driven by a number of complex processes which are deeply interwoven, including mass accretion from nearby (dwarf) systems and the intergalactic medium, mass ejection into the halo and interglactic medium, stellar mass injection into the interstellar medium, star formation, mechanical energy input by stellar winds & supernova explosions, and radiative energy input. These processes are mediated by dust and molecules in an only partially understood way. This complex feedback between stars and the medium they are formed in drives the evolution of galaxies and their observational characteristics. SPICA is set to expand studies of the origin and evolution of the interstellar medium and its role in the evolution of galaxies to the era of vigorous star formation in the Universe at redshifts between 1 and 3. Yet, our understanding of what these observations tell us about what really happens at those epochs will depend very much on our understanding of the microscopic physical and chemical processes and their dependence on the local conditions. These are best studied in the local universe. In order to reap the full benefits of SPICA, a concerted program of key observations is required that study the physics and chemistry of the ISM locally and leverage this to probe the far Universe. | |||||||
| 内容記述 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | 形態: カラー図版あり | |||||||
| 内容記述（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | Physical characteristics: Original contains color illustrations | |||||||
| ISSNONLINE | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 2433-2232 | |||||||
| 資料番号 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | 資料番号: AA1730027037 | |||||||
| レポート番号 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | レポート番号: JAXA-SP-17-010E | |||||||
