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Probing Evolution of Hot Gas and Galaxy Distributions in Galaxy Clusters
https://jaxa.repo.nii.ac.jp/records/5078
https://jaxa.repo.nii.ac.jp/records/5078bbc450ac-838c-42a6-a383-1f96baab3eb8
名前 / ファイル | ライセンス | アクション |
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64574146.pdf (175.9 kB)
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Item type | 会議発表論文 / Conference Paper(1) | |||||
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公開日 | 2015-03-26 | |||||
タイトル | ||||||
言語 | en | |||||
タイトル | Probing Evolution of Hot Gas and Galaxy Distributions in Galaxy Clusters | |||||
言語 | ||||||
言語 | eng | |||||
キーワード | ||||||
言語 | en | |||||
主題Scheme | Other | |||||
主題 | galaxies: clusters: general - X-rays: galaxies: clusters | |||||
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 |
稲田, 直久
× 稲田, 直久× 川原田, 円× 小波, さおり× 三澤, 透× 太田, 一陽× 牧島, 一夫× 高橋, 労太× Inada, Naohisa× Kawaharada, Madoka× Konami, Saori× Gandhi, Poshak× Misawa, Toru× Ota, Kazuaki× Makishima, Kazuo× Takahashi, Rohta |
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著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属 | ||||||
理化学研究所宇宙放射線研究室 | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
著者所属(英) | ||||||
en | ||||||
Cosmic Radiation Laboratory, RIKEN | ||||||
出版者 | ||||||
出版者 | 宇宙航空研究開発機構 | |||||
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 Energetic Cosmos; from Suzaku to ASTRO-H 巻 JAXA-SP-09-008E, p. 380-381, 発行日 2010-02-26 |
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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 | The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan | |||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | The purpose of this work is to answer the question of "how have spatial distributions of components in galaxy clusters evolved over the history of the universe?". It is well known that galaxy clusters consist of dark matter, intergalactic hot gas, and galaxies, and that hot gas has an extended distribution and galaxy components show a morphology-density relation and the Butcher-Oemler effect. However, the origin of these cluster component distributions is still unknown. One simple interpretation is that galaxies have gradually fallen to the cluster centers, with evolution of their color and morphology. If this simple scenario is correct, the relative distributions of galaxies to hot gas should become centrally-concentrated toward lower redshifts. Our exploratory study suggests that galaxies are falling to the cluster center while hot gas is expanding with decreasing redshifts. | |||||
内容記述(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science | |||||
ISSN | ||||||
収録物識別子タイプ | ISSN | |||||
収録物識別子 | 1349-113X | |||||
書誌レコードID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA11984031 | |||||
資料番号 | ||||||
内容記述タイプ | Other | |||||
内容記述 | 資料番号: AA0064574146 | |||||
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-09-008E |