期刊
ASTROPHYSICAL JOURNAL
卷 902, 期 2, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/abb82e
关键词
Galaxy evolution; High-redshift galaxies; Interstellar medium; Molecular gas
资金
- ERC [740246]
- Collaborative Research Centre 956 - Deutsche Forschungsgemeinschaft (DFG) [184018867]
- CASSACA
- FONDECYT [1191124]
- National Science Foundation [AST-1614213, AST-1910107]
- Alexander von Humboldt Foundation through a Humboldt Research Fellowship for Experienced Researchers
- STFC [ST/T000244/1]
- JSPS KAKENHI [JP19K23462]
- Netherlands Organisation for Scientific Research (NWO) [639.042.611]
- Australian Research Council Future Fellowship - Australian Government [FT190100083]
- CONICYT fund CAS-CONICYT Call 2018
We combine the recent determination of the evolution of the cosmic density of molecular gas (H-2) using deep, volumetric surveys, with previous estimates of the cosmic density of stellar mass, star formation rate and atomic gas (Hi), to constrain the evolution of baryons associated with galaxies averaged over cosmic time and space. The cosmic Hiand H(2)densities are roughly equal atz similar to 1.5. The H(2)density then decreases by a factor
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