Resolved and unresolved populations: statistics and synthesis models
classification
🌌 astro-ph
keywords
bumpmodelspopulationssynthesisconfidencecontributiondiagnosticdiagrams
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In this contribution, I present the 90% confidence limits on the diagnostic diagrams of EW(WR bump) and L(WR bump)/L(Hb) ratio vs. EW(Hb) resulting from evolutionary synthesis models that include the statistical dispersion due to finite stellar populations in real star forming regions.
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