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泉研究室
Showing the original Japanese · View translation
銀河の中心で輝く巨大ブラックホールを電波で探る研究室。

AboutAbout the lab
巨大ブラックホールは、どう育つのか。
泉研究室は、
ミリ波・サブミリ波を
超巨大ブラックホールが
泉准教授は
Key terms
- 活動銀河核
- 銀河の
中心が 非常に 明るく 輝いている 天体。 中心の ブラックホールに 物質が 落ち込んで 光る - ミリ波・サブミリ波
- 波長が
ミリメートルや その 十分の 一ほどの 電波。 冷たい ガスや 塵のようすを 見るのに 使う - 超巨大ブラックホール
- 多くの
銀河の 中心に ある、 太陽の 百万倍から 十億倍もの 重さを もつブラックホール
ResearchResearch themes
専門は
*Illustrative image活動銀河核の電波観測
宇宙の
*Illustrative image超巨大ブラックホールの成長
銀河の
*Illustrative image活動銀河核が銀河に与える影響
活動銀河核が、
*Illustrative image爆発的星形成との関係
銀河で
MembersFaculty
- Associate Professor泉 拓磨
VoicesStudent voices
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RelatedLabs similar to 泉研究室
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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: “Artist’s impression of the active galactic nucleus of Messier 77 (eso2203d)” ESO/M. Kornmesser and L. Calçada / CC BY 4.0 (cropped)
- 活動銀河核の
電波観測: “The first three ALMA antennas at the Array Operations Site (AOS) on Chajnantor (ib-alma10)” Iztok Bončina/ALMA (ESO/NAOJ/NRAO) / CC BY 4.0 (cropped) - 超巨大ブラックホールの
成長: “Illustration of Active Galactic Nucleus (2007-agns - accretiondisk torus)” NASA/CXC/Ohio State Univ./J.Eastman et al / Public domain (cropped) - 活動銀河核が
銀河に 与える 影響: “A dust-bound supermassive black hole” ESA/NASA, the AVO project and Paolo Padovani / CC BY 4.0 (cropped) - 爆発的星形成との
関係: “M82 HST ACS 2006-14-a-large web” NASA, ESA, and The Hubble Heritage Team (STScI/AURA) / Public domain (cropped) - Related lab (峰崎岳夫研究室): “NGC 4151 - HST” Judy Schmidt from USA / CC BY 2.0 (cropped)
- Related lab (河野孝太郎研究室): “ALMA antennas on Chajnantor (malin-dsc0027)” ESO/C. Malin / CC BY 4.0 (cropped)
- Related lab (電波天文学グループ(江草研究室)
): “M83 - Southern Pinwheel” (Credit) ESO / CC BY 4.0 (cropped) - Related lab (本間研究室): “Black hole - Messier 87 crop max res” Event Horizon Telescope, uploader cropped and converted TIF to JPG / CC BY 4.0 (cropped)
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