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Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models
When evolutionary synthesis models take into account the stochastic nature of the IMF together with thediscrete number of stars in real stellar clusters, typical output turns to dispersion bands (where real data canbe placed) instead of narrow lines. We present here a qualitative analysis of such di...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2002
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57112089 |
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