THE COSMIC STAR FORMATION HISTORY
A model for calculating the cosmic star formation rate density history in a hierarchical A Cold Dark Matter (ACDM) universe is presented and compared with observations. The role of different astrophysical processes as a function of mass and epoch, and potential shortcomings are discussed.
保存先:
| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2011
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57121297011 |
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