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Paper: Statistical Analysis of PNe in the Galactic Bulge Region
Volume: 424, Proceedings of the 9th International Conference of the Hellenic Astronomical Society
Page: 183
Authors: Akras, S.; Boumis, P.
Abstract: Using new low resolution spectra of Galactic Bulge planetary nebulae (PNe) with the photo-ionization model CLOUDY, the physical parameters of the nebula were determined. In particular, the model predicted the abundances, Te, ne, T and L of the central star etc. The main goal of this work is to investigate possible correlations between the physical parameters of the nebula and their central star by using a statistical tool, the Bayesian theory. These results will help us to understand better the dynamics of the whole bulge region.
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