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Updated: Feb 6, 2026

Transcriptomic Analysis of C. elegans RNA Sequencing Data Through the Tuxedo Suite on the Galaxy Project
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12 億 年 前 の 星爆発 銀河 の 引力 的 に 不安定 な ガス 円盤

K Tadaki1, D Iono2,3, M S Yun4

  • 1National Astronomical Observatory of Japan, Tokyo, Japan. tadaki.ken@nao.ac.jp.

Nature
|August 31, 2018
PubMed
まとめ

初期の宇宙の銀河は 凝縮され 塵に満ちた核心で 星を急速に形成しました 引力的に不安定で 1億年以内にガスを消費します

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