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The Synergy with SPICA and ALMA: for a Robust AGN Diagnostic
https://jaxa.repo.nii.ac.jp/records/3022
https://jaxa.repo.nii.ac.jp/records/30227b26e3df-9754-4be3-95b2-3627e4e78694
名前 / ファイル | ライセンス | アクション |
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AA1730027045.pdf (653.6 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 | The Synergy with SPICA and ALMA: for a Robust AGN Diagnostic | |||||
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 |
泉, 拓磨
× 泉, 拓磨× 河野, 孝太郎× 川勝, 望× Izumi, Takuma× Kohno, Kotaro× Kawakatu, Nozomu |
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著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
東京大学 | ||||||
著者所属 | ||||||
国立高等専門学校機構呉工業高等専門学校 | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
The University of Tokyo | ||||||
著者所属(英) | ||||||
en | ||||||
National Institute of Technology, Kure College | ||||||
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. 211-214, 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 | Here we show the results of our ALMA cycle 0 observation toward the nearby type-1 Seyfert nucleus in NGC 1097. We observed some typical dense gas tracers such as HCN (J=4-3) and HCO+ (J=4-3). We find that the HCN (J=4- 3)/HCO+ (J=4-3) and HCN (J=4-3)/CS (J=7-6) integrated intensity ratios are enhanced in AGNs including NGC 1097 compared to nearby starburst galaxies and Galactic star forming regions. Multi-line/transition analysis of HCN and HCO+ emissions reveal that these lines are emitted from dense (10(exp 4.5) less than or equal to nH2 [cm(exp −3)] less than or equal to 10(exp 6) and hot (70 less than or equal to T(sub kin) [K] less than or equal to 550) regions, and that HCN to HCO+ abundance ratio is high (4-20). We introduce a “high-temperature chemistry” to explain the observed properties. Finally, we briefly discuss the possible future studies with ALMA and SPICA on AGN science. | |||||
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: AA1730027045 | |||||
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 |