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Modelling 30 Doradus in the Large Magellanic Cloud
https://jaxa.repo.nii.ac.jp/records/3096
https://jaxa.repo.nii.ac.jp/records/3096873d9118-bacc-449b-b92b-3db740c26838
名前 / ファイル | ライセンス | アクション |
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AA1730026022.pdf (417.6 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2018-05-16 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Modelling 30 Doradus in the Large Magellanic Cloud | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ISM: dust | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | H II regions | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | infrared: ISM | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | ultraviolet: ISM | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: Magellanic Clouds | |||||
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 |
Saikia, Gautam
× Saikia, Gautam× Singha, Jaikhomba× Shalima, P.× Gogoi, Rupjyoti× Pathak, Amit |
|||||
著者所属(英) | ||||||
en | ||||||
Tezpur University | ||||||
著者所属(英) | ||||||
en | ||||||
Tezpur University | ||||||
著者所属(英) | ||||||
en | ||||||
Regional Institute of Education Mysore | ||||||
著者所属(英) | ||||||
en | ||||||
Tezpur University | ||||||
著者所属(英) | ||||||
en | ||||||
Banaras Hindu 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. 137-140, 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 | The HII regions in the Large Magellanic Cloud (LMC) provide an ideal laboratory to study various processes of dust formation and evolution. The LMC has been targeted by many space-based telescopes, including NASA's Spitzer Space Telescope and more recently, JAXA's AKARI satellite owing to its known distance and nearly face-on orientation with respect to the Milky Way (MW). The highest LMC reddening occurs in the 30 Doradus HII region where the color excess E(sub B-V) reaches a maximum of 0.29. We have done correlation studies in this region between far-ultraviolet (FUV) observations made by the FUSE telescope and infrared (IR) observations made by AKARI in the recent past. In this work, we have attempted to model the FUV scattering by 20 hot stars in the 30 Doradus region within a 1 deg radius. We have chosen an ideal dust distribution facilitating us to study the emission properties around the centre of the nebula. We will also model the IR emission later to conclusively prove the dust properties in the region. | |||||
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: AA1730026022 | |||||
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 |