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山田 智史 研究室
Showing the original Japanese · View translation
ブラックホールと銀河の関係をX線などの多波長観測で探る研究室。
AboutAbout the lab
ブラックホールの働きを、X線と多波長で探る。
山田智史研究室は、
銀河の
最終的には、
東北大学 学際科学フロンティア研究所の
Key terms
- ブラックホールの
風 - ガスの
重力エネルギーが 熱や 運動に 変わる ことで、 周囲の ガスが 吹き飛ば される 現象 - XRISM衛星
- 宇宙の
X線を 観測する 天文衛星。 従来の 装置より 高い 波長分解能で、 X線を 細かく 分けて 測れる - 元素組成比
- ガスなどに
どんな 元素が どんな 割合で 含まれているかを 表した もの。 物質の 由来を 探る 手が かりに なる
ResearchResearch themes
宇宙には
*Illustrative imageブラックホールが銀河に及ぼす影響
巨大ブラックホールは
*Illustrative image物質の運動と元素組成の全体像
ブラックホールに
MembersFaculty
- Assistant Professor山田 智史
VoicesStudent voices
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images.
- Top image: “Chandra X-ray Observatory after release from Space Shuttle Columbia” NASA/STS-93/Cady Coleman / Public domain (cropped)
- ブラックホールが
銀河に 及ぼす影響: “Galactic gas makes a getaway (potw2550a)” ESA/Hubble & NASA, S. Veilleux, J. Wang, J. Greene / CC BY 4.0 (cropped) - 物質の
運動と 元素組成の 全体 像: “M82 Chandra HST Spitzer” NASA/JPL-Caltech/STScI/CXC/UofA/ESA/AURA/JHU / Public domain (cropped) - Related lab (市川 幸平 研究室): “Montage of the Event Horizon Telescope observatories (night) (eso2208-eht-mwg)” ESO/M. Kornmesser. Images of individual telescopes: ALMA: ESO. APEX: ESO. LMT: INAOE Archives. GLT: N. Patel. JCMT: EAO-W. Montgomerie. SMT: D. Harvey. 30m: N. Billot. SPT: Wikipedia. SMA: S. R. Schimpf. NOEMA: IRAM. Kitt Peak: Wikipedia Milky Way: N. Risinger (skysurvey.org) / CC BY 4.0 (cropped)
- Related lab (野田 博文 研究室): “Chandra X-Ray Observatory (noirlab2427c)” NASA/CXC & J.Vaughan / CC BY 4.0 (cropped)
- Related lab (村山 卓 研究室): “Messier83 - Heic1403a” Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: William Blair (Johns Hopkins University) / Public domain (cropped)
- Related lab (児玉 忠恭 研究室): “Galaxy cluster Abell 1689 and distant galaxies ( )” Hubble ESA / CC BY 2.0 (cropped)
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