A new grid of evolutionary synthesis models
classification
🌌 astro-ph
keywords
modelsevolutionaryimportantstarsstellarsynthesisatmospherecluster
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We present new evolutionary synthesis models for Single Stellar Populations covering a wide range in age and metallicity. The most important difference with existing models is the use of NLTE atmosphere models for the hot stars (O, B, WR, post-AGB stars, and planetary nebulae) that have an important impact in the stellar cluster's ionizing spectra.
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