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Dragan Salak 研究室
Showing the original Japanese · View translation
電波望遠鏡で銀河の進化を探る天文学の研究室。

AboutAbout the lab
銀河の誕生と進化を、電波観測で探る。
Dragan Salak研究室は、
宇宙の
分子ガスや
Key terms
- クエーサー
- 銀河の
中心に ある 活動銀河核の うち、 特に 明るく 輝いて 見える 天体 - 活動銀河核
- 銀河の
中心に あり、 銀河全体に 匹敵する ほど 強く 輝く ことが ある 領域 - 分子ガス
- 水素などが
分子の 形に なった 冷たい ガス。 星が 生まれる 材料に なる
NewsLab news
View More ↗ResearchResearch themes
この
*Illustrative image宇宙初期の銀河の誕生と進化
宇宙の
*Illustrative image塵に隠れた銀河とクエーサー
cosmic noon
*Illustrative image近くの銀河の冷たいガス
近傍の
MembersFaculty
- Associate ProfessorDragan Salak
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: “Giant Microwave Radio Telescope” Igoressen / CC0 (cropped)
- 宇宙初期の
銀河の 誕生と 進化: “Building Block Galaxy at Redshift of 5 42 from Hubble Ultra Deep Field Image ( )” NASA, ESA, and N. Pirzkal (STScI/ESA) / Public domain (cropped) - 塵に
隠れた 銀河と クエーサー: “Dusty detail in elliptical galaxy NGC 2768” ESA/Hubble & NASA Acknowledgment: Judy Schmidt / CC BY 4.0 (cropped) - 近くの
銀河の 冷たい ガス: “A galaxy with a glowing heart” ESA/Hubble & NASA Acknowledgements: D. Calzetti (UMass) and the LEGUS Team / CC BY 4.0 (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 (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 (山田 亨 研究室): “Subaru Telescope (6V7A4864-CC)” International Gemini Observatory/NOIRLab/NSF/AURA/ T. Slovinský / CC BY 4.0 (cropped)
- Related lab (田中 秀和 研究室): “Planets in the Making” ALMA (ESO/NAOJ/NRAO); A. Isella; B. Saxton (NRAO/AUI/NSF) / CC BY 4.0 (cropped)
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