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SANHUEZA研究室(Sanhueza Group)
Showing the original Japanese · View translation
大質量星がどうやって生まれるかを、電波望遠鏡で観測する研究室。

AboutAbout the lab
重い星が生まれる現場を、電波でのぞく。
SANHUEZA研究室は、
大質量星は
ALMAや
磁場の
Key terms
- 大質量星
- 太陽より
何倍も 重い星。 一生の 最後に 超新星爆発を 起こし、 中性子星や ブラックホールを 残す - 電波干渉計
- 離れた
場所に 置いた 複数の アンテナの 信号を 合わせ、 巨大な 望遠鏡のように 使う 観測装置 - 初期質量関数
- 生まれた
ばかりの 星たちに ついて、 どの 重さの ものが どれだけ あるかを 表す分布
ResearchResearch themes
大質量星が
*Illustrative image星が生まれる最初の段階
赤外線で
*Illustrative image星形成における磁場の役割
塵から
*Illustrative image連星・降着円盤・流れ込むガス
大質量星の
*Illustrative image星の重さが決まるしくみ
生まれる
MembersFaculty
SANHUEZA研究室の
- Associate ProfessorSANHUEZA PatricioPublications ↗
- Project Assistant ProfessorQiuyi Luo
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RelatedLabs similar to SANHUEZA研究室(Sanhueza Group)
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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: “ALMA view of the star-forming region AFGL 5142 (eso2001b)” ALMA (ESO/NAOJ/NRAO), Rivilla et al. / CC BY 4.0 (cropped)
- 星が
生まれる 最初の 段階: “Infrared Dark Cloud (IRDC) in the W40 region” NASA/Spitzer / Public domain (cropped) - 星形成に
おける 磁場の 役割: “Herschel’s view of the Taurus molecular cloud ESA384012” European Space Agency / CC BY-SA 3.0 igo (cropped) - 連星・降着円盤・
流れ込むガス: “ALMA image of the circumstellar disk AB Aurigae” ALMA (ESO/NAOJ/NRAO)/Tang et al. / CC BY 4.0 (cropped) - 星の
重さが 決まる しく み: “Grand star-forming region R136 in NGC 2070 (infrared, captured by the Hubble Space Telescope)” NASA, ESA, F. Paresce (INAF-IASF), R. O'Connell (University of Virginia) / Public domain (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 (柏川研究室): “Subaru Telescope. Mauna Kea Summit ( )” Robert Linsdell / 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 (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)
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