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観測天文学研究室
Showing the original Japanese · View translation
銀河で星が生まれるしくみを、電波の観測で探る研究室。
AboutAbout the lab
銀河のどこで、星は生まれるのか。
観測天文学研究室は、
星のもとに
赤外線衛星の
Key terms
- 星間ガス
- 星と
星の あいだの 空間に ただよう、 ごく 薄い ガス。 新しい 星が 生まれる 材料に なる - 分子ガス
- 水素などが
分子の 形で 集まった 低温の ガス。 星が 生まれる 場所に 多く、 電波で 観測できる - テラヘルツ波
- 電波と
赤外線の あいだの 周波数の 電磁波。 大気中の 水蒸気に 吸収されやすい
NewsLab news
View More ↗ResearchResearch themes
銀河の
*Illustrative image銀河の星間物質と星の誕生
銀河の
*Illustrative imageCOMING：近傍銀河の分子ガス観測
国立天文台野辺山の
*Illustrative image銀河の形態と進化
銀河が
*Illustrative image南極テラヘルツ望遠鏡計画
筑波大学が
MembersFaculty
- Professor徂徠 和夫
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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. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Nobeyama 45m radiotelescope” Lapinov / CC BY 4.0 (cropped)
- 銀河の
星間物質と 星の 誕生: “APEX view of star formation and cosmic clouds in the Orion Nebula” ESO/Digitized Sky Survey 2 / CC BY 4.0 (cropped) - COMING：近傍銀河の
分子ガス観測: “NGC 7331 (noao-n7331mortfield)” KPNO/NOIRLab/NSF/AURA/Paul Mortfield and Dietmar Kupke/Flynn Haase / CC BY 4.0 (cropped) - 銀河の
形態と 進化: “WISE- Andromeda” NASA/JPL-Caltech/UCLA / Public domain (cropped) - 南極テラヘルツ望遠鏡計画: “South pole telescope nov2009” Amble / CC BY-SA 3.0 (cropped)
- Related lab (理論宇宙物理学研究室): “The spiral galaxy NGC 941 photographed by the Hubble Space Telescope” ESA/Hubble & NASA, C. Kilpatrick / Public domain (cropped)
- Related lab (科学技術コミュニケーション研究室): “Manitoba Museum Planetarium” TMMCommunications / CC BY-SA 4.0 (cropped)
- Related lab (医療基礎物理学研究室): “Cyclotron with glowing beam” 作者不詳 / Public domain (cropped)
- Related lab (量子物性物理学研究室): “Thin section scan crossed polarizers Siilinjärvi R edit” kallerna / CC BY-SA 4.0 (cropped)
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