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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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H I 銀河の集合体からの21センチメートルの放射は,平均赤道偏移1で

Aditya Chowdhury1, Nissim Kanekar2, Jayaram N Chengalur1

  • 1National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune, India.

Nature
|October 15, 2020
PubMed
まとめ

科学者は銀河の原子水素 (H I) ガス質量を赤偏移1で測定した. このガスの質量は恒星質量に似ており 恒星形成を1〜20億年しか維持できず ガス蓄積不足が宇宙の恒星形成の減少を引き起こしたことを示唆している.

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