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在年轻宇宙中的正常大质量恒星形成星系中,高分子气体分数存在

L J Tacconi1, R Genzel, R Neri

  • 1Max-Planck-Institut für extraterrestrische Physik (MPE), Giessenbachstr. 1, 85748 Garching, Germany. linda@mpe.mpg.de

Nature
|February 12, 2010
PubMed
概括

遥远的星系富含分子气体,为快速恒星形成提供了燃料. 这种气体含量明显高于当今星系的含量,这表明早期宇宙中存在连续的气体补充机制.

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