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- W199473 abstract "Evolutionary synthesis models have been used to study the physical properties of unresolved populations in a wide range of scenarios. Unfortunately, their self-consistency is difficult to test and there are some theoretical open questions without an answer: (1) The change of the homology relations assumed in the computation of isochrones due to the effect of stellar winds (or rotation) and the discontinuities in the stellar evolution are not considered. (2) There is no consensus about how the isochrones must be integrated. (3) The discreteness of the stellar populations (that produce an intrinsic statistical dispersion) usually are not taken into account, and model results are interpreted in a deterministic way instead of a statistical one. The objective of this contribution is to present some inconsistencies in the computation and some cautions in the application of the results of such codes.KeywordsStars: evolutionGalaxies: stellar contentopen clusters and associations: general" @default.
- W199473 created "2016-06-24" @default.
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- W199473 date "2003-01-01" @default.
- W199473 modified "2023-09-25" @default.
- W199473 title "On the Self-Consistency of Evolutionary Synthesis Models" @default.
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- W199473 doi "https://doi.org/10.1007/978-94-017-3315-1_119" @default.
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