Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models
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| Natura: | Artículo científico |
| Lingua: | en |
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Universidad Nacional Autónoma de México
2002
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| _version_ | 1876429829764546560 |
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| author | M. Cerviño |
| author_facet | M. Cerviño |
| contents | Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models M. Cerviño V. Luridiana Física, Astronomía y Matemáticas GALAXIES: EVOLUTION 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 dispersion in the SN rate,the kinetic energy and the 14N/12C ratio for di erent amounts of mass transformed into stars. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112089 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| format | Artículo científico |
| id | redalyc_57112089 |
| institution | Redalyc |
| language | en |
| publishDate | 2002 |
| publisher | Universidad Nacional Autónoma de México |
| spellingShingle | Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models M. Cerviño Física, Astronomía y Matemáticas GALAXIES: EVOLUTION Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models M. Cerviño V. Luridiana Física, Astronomía y Matemáticas GALAXIES: EVOLUTION 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 dispersion in the SN rate,the kinetic energy and the 14N/12C ratio for di erent amounts of mass transformed into stars. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112089 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12 |
| title | Confidence limits of sn, kinetic energy and chemical yields in evolutionary synthesis models |
| topic | Física, Astronomía y Matemáticas GALAXIES: EVOLUTION |
| url | https://www.redalyc.org/articulo.oa?id=57112089 |