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.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.063 seconds