Gamow, G. (1948). «The Origin of Elements and the Separation of Galaxies». Phys. Rev. 74 (4): 505–6. Bibcode:1948PhRv...74..505G. doi:10.1103/PhysRev.74.505.2Gamow, G. (30 de outubro de 1948). «The Evolution of the Universe». Nature. 162 (4122): 680–2. Bibcode:1948Natur.162..680G. PMID18893719. doi:10.1038/162680a0Alpher, R.A. (1948). «A Neutron-Capture Theory of the Formation and Relative Abundance of the Elements». Phys. Rev. 74 (11): 1577–89. Bibcode:1948PhRv...74.1577A. doi:10.1103/PhysRev.74.1577 Alpher and Herman first estimated the temperature of the cosmic microwave background as 5° K, and two years later they re-estimated it as 28° K.
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Gamow, G. (1948). «The Origin of Elements and the Separation of Galaxies». Phys. Rev. 74 (4): 505–6. Bibcode:1948PhRv...74..505G. doi:10.1103/PhysRev.74.505.2Gamow, G. (30 de outubro de 1948). «The Evolution of the Universe». Nature. 162 (4122): 680–2. Bibcode:1948Natur.162..680G. PMID18893719. doi:10.1038/162680a0Alpher, R.A. (1948). «A Neutron-Capture Theory of the Formation and Relative Abundance of the Elements». Phys. Rev. 74 (11): 1577–89. Bibcode:1948PhRv...74.1577A. doi:10.1103/PhysRev.74.1577 Alpher and Herman first estimated the temperature of the cosmic microwave background as 5° K, and two years later they re-estimated it as 28° K.
Gamow, G. (1948). «The Origin of Elements and the Separation of Galaxies». Phys. Rev. 74 (4): 505–6. Bibcode:1948PhRv...74..505G. doi:10.1103/PhysRev.74.505.2Gamow, G. (30 de outubro de 1948). «The Evolution of the Universe». Nature. 162 (4122): 680–2. Bibcode:1948Natur.162..680G. PMID18893719. doi:10.1038/162680a0Alpher, R.A. (1948). «A Neutron-Capture Theory of the Formation and Relative Abundance of the Elements». Phys. Rev. 74 (11): 1577–89. Bibcode:1948PhRv...74.1577A. doi:10.1103/PhysRev.74.1577 Alpher and Herman first estimated the temperature of the cosmic microwave background as 5° K, and two years later they re-estimated it as 28° K.
