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- W1975694570 abstract "It is often stated that there are insufficient baryons in galaxies and clusters to satisfy the constraints imposed by primordial nucleosynthesis. Here a recent analysis of the baryon content of the Universe by Persic & Salucci is reconsidered, with the aim of estimating the uncertainties induced in the results by uncertainties in the galaxy population parameters used. The estimates of Ω b turn out to be dependent upon poorly constrained input parameters, in particular the luminosity-function slope parameter, α, and the mass-to-light ratio index, η. It is found that with different, but allowed, choices of input parameters − which admit of large numbers of low-luminosity galaxies − a value of the baryon density consistent with standard primordial nucleosynthesis (0.040≤Ω b h 50 2 ≤0.064) can be recovered" @default.
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- W1975694570 date "1994-03-01" @default.
- W1975694570 modified "2023-10-18" @default.
- W1975694570 title "On the baryon content of the Universe" @default.
- W1975694570 doi "https://doi.org/10.1093/mnras/267.1.13" @default.
- W1975694570 hasPublicationYear "1994" @default.
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