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  2. 光中的分子气体推动了巨大的星系团在高红移的增长
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  2. 光中的分子气体推动了巨大的星系团在高红移的增长

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光中的分子气体推动了巨大的星系团在高红移的增长

B H C Emonts1, M D Lehnert2, M Villar-Martín3,4

  • 1Centro de Astrobiología (Consejo Superior de Investigaciones Científicas-Instituto Nacional de Técnica Aerospacial), Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Madrid, Spain. bjornemonts@gmail.com.

Science (New York, N.Y.)
|December 10, 2016

在PubMed 上查看摘要

概括
此摘要是机器生成的。

巨大的星系从巨大的分子气体库中形成. 这种气体在星系间介质中存在,

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科学领域:

  • 宇宙进化和星系的形成
  • 天体物理学和观测宇宙学

背景情况:

  • 巨大的星系主要存在于星系团中.
  • 这些巨大的星系的形成机制尚未完全理解.

研究的目的:

  • 探究蜘蛛网星系中燃烧恒星形成的气体储备,
  • 了解星系间气体在巨型星系团形成中的作用.

主要方法:

  • 使用敏感的一氧化碳观测.
  • 在原团环境中分析了分子气体分布和速度分散.

主要成果:

  • 在原始集群中发现了大量的分子气体.
  • 确定大部分的气体存在于低速度分散的星系之间.
  • 表明该气体是银河系中富含物质的一部分.

结论:

  • 蜘蛛网星系是从一个大量的分子气体储备中形成的.
  • 这种星系间气体可能为星系的星系形成提供燃料.
  • 巨大的星系群可能由高红移的循环气体形成.