Confidence Limits of SN, Kinetic Energy and Chemical Yields in Evolutionary Synthesis Models

Bibcode
2002RMxAC..12..240C
Cerviño, M.; Luridiana, V.
Bibliographical reference

Ionized Gaseous Nebulae, a Conference to Celebrate the 60th Birthdays of Silvia Torres-Peimbert and Manuel Peimbert, Mexico City, November 21-24, 2000 (Eds. W. J. Henney, J. Franco, M. Martos, & M. Peña) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 12, pp. 240-241 (2002) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
2
2002
Number of authors
2
IAC number of authors
0
Citations
1
Refereed citations
1
Description
When evolutionary synthesis models take into account the stochastic nature of the IMF together with the discrete number of stars in real stellar clusters, typical output turns to dispersion bands (where real data can be 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 different amounts of mass transformed into stars.
Type
Non-refereed
Galaxies

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