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What makes Ultra Luminous Infrared Galaxies shine? Properties and environments of ULIRGs from the AKARI Deep Field-South
https://jaxa.repo.nii.ac.jp/records/3143
https://jaxa.repo.nii.ac.jp/records/314370e70a69-9fff-4106-beb9-af463df7e4d5
名前 / ファイル | ライセンス | アクション |
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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 | What makes Ultra Luminous Infrared Galaxies shine? Properties and environments of ULIRGs from the AKARI Deep Field-South | |||||
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 |
Bankowicz, Malgorzata
× Bankowicz, Malgorzata× Pollo, Agnieszka× Malek, Katarzyna× 竹内, 努× Burgarella, Denis× Buat, Veronique× Malkan, Matt× Herzig, Aleksander× Bankowicz, Malgorzata× Pollo, Agnieszka× Malek, Katarzyna× Takeuchi, Tsutomu× Burgarella, Denis× Buat, Veronique× Malkan, Matt× Herzig, Aleksander |
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著者所属 | ||||||
Astronomical Observatory of the Jagiellonian University | ||||||
著者所属 | ||||||
Astronomical Observatory of the Jagiellonian University : National Centre for Nuclear Research, Poland | ||||||
著者所属 | ||||||
National Centre for Nuclear Research, Poland | ||||||
著者所属 | ||||||
名古屋大学 | ||||||
著者所属 | ||||||
Aix-Marseille Universite | ||||||
著者所属 | ||||||
Aix-Marseille Universite | ||||||
著者所属 | ||||||
University of California, Los Angeles | ||||||
著者所属(英) | ||||||
en | ||||||
Astronomical Observatory of the Jagiellonian University | ||||||
著者所属(英) | ||||||
en | ||||||
Astronomical Observatory of the Jagiellonian University : National Centre for Nuclear Research, Poland | ||||||
著者所属(英) | ||||||
en | ||||||
National Centre for Nuclear Research, Poland | ||||||
著者所属(英) | ||||||
en | ||||||
Nagoya University | ||||||
著者所属(英) | ||||||
en | ||||||
Laboratoire d'Astrophysique de Marseille : OAMP : Universite Aix-Marseille : The National Center for Scientific Research (CNRS) | ||||||
著者所属(英) | ||||||
en | ||||||
Laboratoire d'Astrophysique de Marseille : OAMP : Universite Aix-Marseille : The National Center for Scientific Research (CNRS) | ||||||
著者所属(英) | ||||||
en | ||||||
University of California, Los Angeles | ||||||
著者所属(英) | ||||||
en | ||||||
Astronomical Observatory of the Jagiellonian 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: The Cosmic Wheel and the Legacy of the AKARI archive: from galaxies and stars to planets and life 巻 JAXA-SP-17-009E, p. 347-350, 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 | Brackets Ultra brackets Luminous Infrared Galaxies (brackets U brackets LIRGs) are a rare class of galaxies whose exact mechanisms of activity and very high dust luminosity are still under debate, with the mixed role of galaxy mergers, starburst and Active Galactic Nucleus (AGN) to be clarified. For 39 brackets U brackets LIRGs discovered in the AKARI Deep Field-South (Malek et al. 2017) we analyzed their properties and found that ULIRGs are more commonly associated with edge-on (Type 2) AGNs than LIRGs which may point out to the geometric factor in whether we detect an object as a ULIRG or LIRG. Next, we attempted to evaluate galactic density in their vicinity based on the Digital Sky Survey (DSS) data and dedicated follow-up observations by the South African Astronomical Observatory (SAAO) telescopes. We concluded that ULIRGs prefer environments with high but not extreme density while LIRGs are more often found also in denser environments. It may imply that ULIRGs appear most often in the environment of the cluster outskirts, where galaxy mergers are the most probable, and it supports the hypothesis that mergers play the crucial role in their activation. | |||||
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: AA1730026069 | |||||
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 |