NGC 6553 is a metal-rich globular cluster that formed in situ in the Galactic bulge, shown by its abundance patterns, multiple populations, and chemical DNA tests.
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3 Pith papers cite this work. Polarity classification is still indexing.
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2026 3verdicts
UNVERDICTED 3representative citing papers
Monte Carlo tests with mock clusters show that fitting Gaia-like photometry with isochrones from different stellar codes produces biases of 0.6 to 1.5 in ΔY/ΔZ unless identical models are used for generation and fitting.
Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.
citing papers explorer
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The Bulge Cluster Origin (BulCO) survey with CRIRES at the ESO-VLT: a chemical screening of the Globular Cluster NGC 6553
NGC 6553 is a metal-rich globular cluster that formed in situ in the Galactic bulge, shown by its abundance patterns, multiple populations, and chemical DNA tests.
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A critical analysis of main-sequence fitting in open clusters to derive the helium-to-metal enrichment ratio $\Delta Y/\Delta Z$
Monte Carlo tests with mock clusters show that fitting Gaia-like photometry with isochrones from different stellar codes produces biases of 0.6 to 1.5 in ΔY/ΔZ unless identical models are used for generation and fitting.
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Investigating the impact of Solar Fusion III reaction rates on helioseismic constraints and solar neutrino fluxes
Solar models with Solar Fusion III reaction rates show slight improvement in helioseismic agreement but lower predicted beryllium, boron, and CNO neutrino fluxes, with rate uncertainties insufficient to match observations.