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- W2892059810 abstract "The abundance of alpha elements and iron in stars of globular clusters (GCs) shows the composition of the gaseous medium, in which they have been formed. In this paper, we discuss a possibility to consider dense clouds of circumgalactic gas (partial Lyman limit systems and Lyman limit systems) observed in the 100–130 kpc neighbourhood of galaxies at redshifts of |$rm 0.1lt zlt 1.1$| as being the residual parts of clouds, in which globular clusters have been formed. Conclusions have been drawn based on statistical analysis of the abundance of magnesium and iron in GCs and in circumgalactic clouds and on the spatial location of objects of both types." @default.
- W2892059810 created "2018-09-27" @default.
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- W2892059810 date "2018-09-05" @default.
- W2892059810 modified "2023-09-24" @default.
- W2892059810 title "On the relationship between metallicity distributions of globular clusters and of circumgalactic gas" @default.
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- W2892059810 doi "https://doi.org/10.1093/mnras/sty2419" @default.
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