Why does the Milky Way have a metallicity floor?
Britton D. Smith, Brian W. O'Shea, Sadegh Khochfar, Matthew J. Turk,, John H. Wise, Michael L. Norman

TL;DR
This paper investigates the origin of the Milky Way's metallicity floor, proposing it results from metal-enriched star formation in early minihalos, supported by cosmological simulations and a hybrid gas evolution model.
Contribution
It introduces a hybrid one-zone model that accurately reproduces gas evolution in minihalos, linking metallicity levels to the onset of gravitational instability and star formation.
Findings
Metallicity of ~10^{-3.7} Z_sun enables gas collapse in minihalos.
Absence of metals stabilizes gas against collapse as halos grow.
Metal enrichment triggers star formation at the metallicity floor.
Abstract
The prevalence of light element enhancement in the most metal-poor stars is potentially an indication that the Milky Way has a metallicity floor for star formation around 10 Z. We propose that this metallicity floor has its origins in metal-enriched star formation in the minihalos present during the Galaxy's initial formation. To arrive at this conclusion, we analyze a cosmological radiation hydrodynamics simulation that follows the concurrent evolution of multiple Population III star-forming minihalos. The main driver for the central gas within minihalos is the steady increase in hydrostatic pressure as the halos grow. We incorporate this insight into a hybrid one-zone model that switches between pressure-confined and modified free-fall modes to evolve the gas density with time according to the ratio of the free-fall and sound-crossing timescales. This model is…
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Taxonomy
TopicsHistory and Developments in Astronomy
