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astro-ph2000
Confidence levels of evolutionary synthesis models
M. Cervino, V. Luridiana, F. J. Castander
The stochastic nature of the IMF in young stellar clusters implies that clusters of the same mass and age do not present the same unique values of their observed parameters. Instea…
astro-ph2000
Energy implications of temperature fluctuations in photoionized plasma
L. Binette, V. Luridiana
We quantify the energy radiated through all the collisionally excited lines in a photoionized nebula which is permeated by temperature fluctuations. We assume that these correspond…