Investigating black hole accretion disks as potential polluter sources for the formation of enriched stars in globular clusters

Open Access

Fig. 3.

Illustration of the evolution of the enrichment timescale, τ_e, as a function of the parameter ξ. The lines are colored according to the temperature (in MK). The higher is ξ, the more enriched is the final composition in the corresponding chemical element, here ²⁷Al. The enrichment timescale is directly dependent on the temperature.

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