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- W1535815223 abstract "Clusters of galaxies allow a direct estimate of the metallicity and metal production yield on the largest scale so far. It is argued that cluster metallicity ($sim 1/3$ solar) should be taken as representative of the low-$z$ universe as a whole. There is now compelling evidence that the bulk of stars not only in cluster ellipticals but also in field ellipticals and bulges formed at high redshifts ($zgsim 3$). Since such stars account for at least $sim 30%$ of the baryons now locked into stars, it is argued that at least 30% of stars and metals formed before $zsimeq 3$, and correspondingly the metallicity of the universe at $z=3$ is predicted to be $sim 1/10$ solar. This requires the cosmic star formation rate to run at least flat from $zsim 1$ to $sim 5$, which appears to agree with the most recent derect determinations of the star formation rate in Lyman-break galaxies." @default.
- W1535815223 created "2016-06-24" @default.
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- W1535815223 date "1998-10-20" @default.
- W1535815223 modified "2023-09-27" @default.
- W1535815223 title "Hints on Galaxy Formation from the Metal Content of Galaxy Cluster and Other Fossil Evidence" @default.
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- W1535815223 hasPublicationYear "1998" @default.
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