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電波天文学グループ（江草研究室）
Showing the original Japanese · View translation
渦を巻く銀河のガスの動きと星の誕生を、電波で調べる研究室。
AboutAbout the lab
渦を巻く銀河のガスを、電波で読み解く。
江草研究室は、
天文学教育研究センターの
電波や
近くの
Key terms
- 星間物質
- 星と
星の あいだに 広がる ガスやちり。 新しい 星を つくる 材料に なる - 分子雲
- 水素などが
分子の 形で 濃く 集まった ガスの 雲。 星が 生まれる 場所に なる - アルマ
- チリの
アタカマ高地に ある 電波望遠鏡。 多数の アンテナを 組み合わせて ミリ波・サブミリ波を 観測する
NewsLab news
View More ↗ResearchResearch themes
電波天文学グループの
*Illustrative image渦状銀河・棒渦状銀河のガス
渦状銀河や
*Illustrative image分子雲の統計的研究
近くの
*Illustrative image突発天体が起きた銀河
γ線バーストや
MembersFaculty
江草研究室が
- Associate Professor江草 芙実Publications ↗
- Assistant Professor諸隈 佳菜
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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: “M83 - Southern Pinwheel” (Credit) ESO / CC BY 4.0 (cropped)
- 渦状銀河・棒渦状銀河の
ガス: “The NGC 1300 galaxy as seen with ALMA (ngc1300-alma-cc)” ESO/ALMA (ESO/NAOJ/NRAO)/PHANGS / CC BY 4.0 (cropped) - 分子雲の
統計的研究: “The NGC 4254 galaxy as seen with ALMA (ngc4254-alma-cc)” ESO/ALMA (ESO/NAOJ/NRAO)/PHANGS / CC BY 4.0 (cropped) - 突発天体が
起きた 銀河: “Fast Radio Burst 180916 Host Galaxy (unannotated) (noirlab2002b)” Gemini Observatory/NOIRLab/NSF/AURA / CC BY 4.0 (cropped) - Related lab (泉研究室): “Artist’s impression of the active galactic nucleus of Messier 77 (eso2203d)” ESO/M. Kornmesser and L. Calçada / CC BY 4.0 (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 (柏川研究室): “Subaru Telescope. Mauna Kea Summit ( )” Robert Linsdell / CC BY 2.0 (cropped)
- Related lab (嶋作研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
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