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The AKARI Spectra of Luminous Infrared Galaxies in the Local Universe
https://jaxa.repo.nii.ac.jp/records/3111
https://jaxa.repo.nii.ac.jp/records/311176c2fea2-8598-41a5-af2d-9dee55edf028
名前 / ファイル | ライセンス | アクション |
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AA1730026037.pdf (4.7 MB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-18 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | The AKARI Spectra of Luminous Infrared Galaxies in the Local Universe | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: active | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: starburst | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared: galaxies | |||||
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 |
稲見, 華恵
× 稲見, 華恵× 松原, 英雄× Armus, Lee× Charmandaris, Vassilis× DiazSantos, Tanio× Surace, Jason× Stierwalt, Sabrina× GOALS Team× Inami, Hanae× Matsuhara, Hideo× Armus, Lee× Charmandaris, Vassilis× DiazSantos, Tanio× Surace, Jason× Stierwalt, Sabrina× GOALS Team |
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著者所属 | ||||||
Universite de Lyon : Universite de Lyon 1 : Ens de Lyon : CNRS : Centre de Recherche Astrophysique de Lyon (CRAL) | ||||||
著者所属 | ||||||
宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS) | ||||||
著者所属 | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
著者所属 | ||||||
Institute for Astronomy, Astrophysics, Space Applications & Remote Sensing, National Observatory of Athens : University of Crete | ||||||
著者所属 | ||||||
Universidad Diego Portales | ||||||
著者所属 | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
著者所属 | ||||||
University of Virginia : National Radio Astronomy Observatory, USA | ||||||
著者所属 | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
著者所属(英) | ||||||
en | ||||||
Universite de Lyon : Universite de Lyon 1 : Ens de Lyon : CNRS : Centre de Recherche Astrophysique de Lyon (CRAL) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) | ||||||
著者所属(英) | ||||||
en | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
著者所属(英) | ||||||
en | ||||||
Institute for Astronomy, Astrophysics, Space Applications & Remote Sensing, National Observatory of Athens : University of Crete | ||||||
著者所属(英) | ||||||
en | ||||||
Universidad Diego Portales | ||||||
著者所属(英) | ||||||
en | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
著者所属(英) | ||||||
en | ||||||
University of Virginia : National Radio Astronomy Observatory, USA | ||||||
著者所属(英) | ||||||
en | ||||||
Infrared Processing and Analysis Center, California Institute of Technology (Caltech) (IPAC) | ||||||
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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 221-224, 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) | ||||||
内容記述タイプ | Other | |||||
内容記述 | 第4回「あかり」国際会議 (2017年10月17-20日. 東京大学), 文京区, 東京 | |||||
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 | The 4th AKARI International Conference: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life (October 17-20, 2017. The University of Tokyo), Bunkyo-ku, Tokyo, Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | We have combined AKARI 2.5-5 micrometers and Spitzer 5.2-38 micrometers spectra of 145 local luminous infrared galaxies (LIRGs) drawn from the Great Observatories All-sky LIRG Survey (GOALS). The equivalent widths (EQWs) of the polycyclic aromatic hydrocarbon (PAH) emission features detected at 3.3 micrometers and 6.2 micrometers, the two most commonly used indicators for classifying the central energy sources (starburst or active galactic nucleus, AGN), do not appear to be linearly correlated. Moreover, about 30% of the AGN-dominated galaxies classified by the 3.3 micrometers PAH EQW are, on the contrary, suggested to be starburst-dominated galaxies by the 6.2 micrometers PAH EQW. We find that the Spitzer spectra of the sources with low 3.3 micrometers PAH EQW but high 6.2 micrometers PAH EQW are remarkably similar to the spectra of pure starburst sources. However, their 2-5 micrometers continua in AKARI spectra are much bluer, suggesting that the continuum is dominated by stellar emission rather than hot dust emission. Based on these results, we suggest a revised diagnostic using the 3.3 micrometers PAH EQW and the continuum color. We also report on a possible diagnostic with the capabilities of the James Webb Space Telescope (JWST) based on the results from the AKARI and Spitzer data. | |||||
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: AA1730026037 | |||||
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-17-009E |