11 papers · 1 filter
Physical conditions in NGC 6543 from ISO and HST data and the pitfalls of temperature maps
V. Luridiana, E. Perez, M. Cervino
We determine the physical conditions in NGC 6543, obtaining two different estimates of the electron temperature (T_e) and one estimate of the electron density (N_e). The electron t…
Statistical Synthesis Models
M. Cervino, V. Luridiana
In this contribution we evaluate the minimal cluster mass for which the effects of an incomplete sampling of the Initial Mass Function (IMF) cannot be neglected. This minimal clust…
A multiwavelength vision of star forming regions: What does lambda_1 know about lambda_2?
M. Cervino
In this contribution I show the physical limitations to the application of standard synthesis models from 0 to 10 Gyr. I also present the multiwavelength spectrum (from gamma-rays…
Resolved and unresolved populations: statistics and synthesis models
M. Cervino
In this contribution, I present the 90% confidence limits on the diagnostic diagrams of EW(WR bump) and L(WR bump)/L(Hb) ratio vs. EW(Hb) resulting from evolutionary synthesis mode…
Statistics and multiwavelength synthesis models: towards a new generation of synthesis models
M. Cervino
In this contribution I present my current work in a new generation of evolutionary synthesis models that compute the multiwavelength energy distribution (from gamma-rays to radio)…
On some Uncertainties in Evolutionary Synthesis Models
M. Cervino, D. Valls--Gabaud
Ranging from track interpolation techniques through model atmospheres to the stochastic nature of the IMF, there are many uncertainties which need to be taken into account when mod…