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Far-Infrared Line Deficits in Ultraluminous Infrared Galaxies
https://jaxa.repo.nii.ac.jp/records/3002
https://jaxa.repo.nii.ac.jp/records/3002be4a814e-d119-425d-8ba8-be2976ba3029
名前 / ファイル | ライセンス | アクション |
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AA1730027025.pdf (391.6 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-01 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Far-Infrared Line Deficits in Ultraluminous Infrared Galaxies | |||||
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 |
Farra, D.
× Farra, D.× Lebouteiller, V.× Rigopoulou, D.× BernardSalas, J.× Efstathiou, A.× GonzalezAlfonso, E.× The HERUS team |
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著者所属(英) | ||||||
en | ||||||
Le Centre CEA de Saclay | ||||||
著者所属(英) | ||||||
en | ||||||
Le Centre CEA de Saclay | ||||||
著者所属(英) | ||||||
en | ||||||
University of Oxford | ||||||
著者所属(英) | ||||||
en | ||||||
The Open University | ||||||
著者所属(英) | ||||||
en | ||||||
European University Cyprus | ||||||
著者所属(英) | ||||||
en | ||||||
Universidad de Alcala | ||||||
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. 113-115, 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 | We study the origin of the [O I] 63, [N II] 122, [O I] 145, and [C II] 158 line deficits in z less than 0.3 Ultraluminous Infrared Galaxies, using data from Herschel. The line deficits are consistent with arising from increased quantities of dust in HII regions, but part of the [C II] deficit may arise from an additional mechanism, plausibly increased grain charging. We briefly discuss some implications from these results for SPICA. | |||||
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: AA1730027025 | |||||
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 |