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Pre-Galactic

In recent years, intensive efforts have been made to improve the determination of the pre-Galactic helium abundance (generally assumed to be the same as FP) and AF/AZ from observations of extragalactic H II regions. Advantages of this method are ... [Pg.141]

Figure 8 also shows the evolution of the Li abundance in a standard model of galactic chemical evolution. In the case of Li, new data [77, 78, 79, 80, 81, 82] lie a factor - 1000 above the BBN predictions [83], and fail to exhibit the dependence on metallicity expected in models based on nucleosynthesis by Galactic cosmic rays [84, 85, 86]. On the other hand, the Li abundance may be explained by pre-Galactic Population-Ill stars, without additional overproduction of Li [87, 88]. Some exotic solutions to both lithium problems involving particle decays in the early universe have been proposed [89, 90, 91, 92, 93,94, 95,96,97,98], but that goes beyond the scope of this review. [Pg.32]

Table 2. Pre-Galactic concentrations in the Alamosa River below the mouth of Wightman Fork (AR 45.4)... Table 2. Pre-Galactic concentrations in the Alamosa River below the mouth of Wightman Fork (AR 45.4)...
Monte Carlo Simulation of Pre-Galactic and Pre-Mining Chemistry... [Pg.158]

The pre-Galactic water quality for copper and zinc during 11 (Figures 6-7) likely represent the worst-case seasonal values in the Alamosa downstream of Wightman Fork. Chopper concentrations show a pronounced effect of the iron oxide partitioning in the water column and well as reduced transport of ct per due to retention by stream sediments. [Pg.159]

Concentrations of dissolved and total zinc were nearly identical and indicated the limited partitioning of zinc to the iron oxides at pH conditions in the Alamosa River (<7.0) for the pre-Galactic scenario. While the concentration of total copper is reduced by 82% firom Wightman Fork to Terrace Reservoir through combined adsorption (to bed sediments) and dilution, the zinc concentration is reduced 1 47%. Zinc and copper are both removed to the bed sediments, although zinc is removed less efficiently. If pH were in the range of 7.S-8.0 in the system, both zinc and copper adsorption would be enhanced and the associated dissolved metal in the water column would be decreased further. [Pg.160]

Figure 6. Simulated Pre-Galactic copper concentrations during fall. Figure 6. Simulated Pre-Galactic copper concentrations during fall.
Medine, A. J. Technical Assessment of Pre-Mining and Pre-Galactic Water Quality for Wightman Fork and the Alamosa River. USEPA, National Risk Management Research Laboratory, Cincinnati, OH, 1997. [Pg.163]


See other pages where Pre-Galactic is mentioned: [Pg.355]    [Pg.356]    [Pg.227]    [Pg.303]    [Pg.323]    [Pg.115]    [Pg.16]    [Pg.81]    [Pg.87]    [Pg.96]    [Pg.101]    [Pg.110]    [Pg.172]    [Pg.192]    [Pg.201]    [Pg.249]    [Pg.289]    [Pg.203]    [Pg.151]    [Pg.154]    [Pg.158]    [Pg.158]    [Pg.159]    [Pg.159]    [Pg.161]    [Pg.161]    [Pg.162]   
See also in sourсe #XX -- [ Pg.159 ]




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Galactal

Galactic

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