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小林・新納研究室
Showing the original Japanese · View translation
短い時間で明るさを変える天体を、木曽の望遠鏡で追う研究室。
AboutAbout the lab
一瞬の光の変化を、見逃さない。
小林・新納研究室は、
東大木曽観測所の
重力波や
可視光の
Key terms
- シュミット望遠鏡
- 鏡と
補正板を 組み合わせ、 一度に 広い範囲の 空を 撮れるように した 望遠鏡 - FRB
- 数ミリ秒だけ強い
電波が 届く、 正体の よく 分かっていない 宇宙の 現象。 高速電波バースト - 質量降着
- 星の
まわりの ガスやちりが、 重力に 引かれて星の 表面に 落ち込んでいく こと
ResearchResearch themes
木曽観測所の
*Illustrative image重力波に対応して光る天体
KAGRA などの
*Illustrative imageFRBに対応する天体の探査
数ミリ秒の
*Illustrative image若い星の明るさの変化
生まれてから
*Illustrative image近くの星形成領域と若い星団
おうし座の
MembersFaculty
小林・新納研究室には、
- Associate Professor小林 尚人Publications ↗
- Assistant Professor新納 悠
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: “Orion Nebula - Hubble 2006 mosaic 18000” NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team / Public domain (cropped)
- 重力波に
対応して 光る 天体: “Artist’s impression of merging neutron stars” ESO/L. Calçada/M. Kornmesser / CC BY 4.0 (cropped) - FRBに
対応する 天体の 探査: “Artist’s impression of a record-breaking fast radio burst (eso2317a)” ESO/M. Kornmesser / CC BY 4.0 (cropped) - 若い星の
明るさの 変化: “T Tauri in NGC 1555 (noao-ttau)” T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOIRLab/NSF/AURA / CC BY 4.0 (cropped) - 近くの
星形成領域と 若い 星団: “Taurus molecular cloud (eso1209ec)” ESO / CC BY 4.0 (cropped) - Related lab (宮田隆志研究室): “Wolf-Rayet 140 (Webb-MIRI)” NASA/ESA/CSA/STScl/JPL-Caltech / Public domain (cropped)
- Related lab (本原顕太郎研究室): “Hubble-ultra-deep-field-20091208-WFC3-IR-full” NASA / Public domain (cropped)
- Related lab (嶋作研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
- Related lab (酒向重行研究室): “The Test-Bed Telescope 2 dome at night (eso2107h)” F. Ocaña/J. Isabel/Quasar SR / CC BY 4.0 (cropped)
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