Hostname: page-component-7bb8b95d7b-qxsvm Total loading time: 0 Render date: 2024-09-30T05:23:30.452Z Has data issue: false hasContentIssue false
  • English
  • Français

Physical parameters and chemical abundances of Planetary Nebulae in the large Magellanic Cloud

Published online by Cambridge University Press:  25 May 2016

R. E. Carlos Reyes ,
J. E. Steiner  and
F. Elizalde
R. E. Carlos Reyes
Affiliation:
1Instituto Astronômico e Geofísico da USP, Brazil 2Divisão de Astrofísica - INPE, Brazil
J. E. Steiner
Affiliation:
1Instituto Astronômico e Geofísico da USP, Brazil
F. Elizalde
Affiliation:
2Divisão de Astrofísica - INPE, Brazil

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

In the present work we have computed the physical parameters and chemical abundances for 45 planetary nebulae (PN) in the Large Magellanic Cloud (LMC) using the photoionization code CLOUDY, developed by Ferland (1993). CLOUDY is used as a subroutine in the code DIANA, developed by Elizalde & Steiner (1996), which minimises indices that measures the difference between the calculated and real nebula.

Type
VIII. Planetary Nebulae in Extragalactic Systems
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 471
Copyright
Copyright © Kluwer 1997 

References

Vassiliadis, et al., 1996, ApJS, 105, 375.Google Scholar
Elizalde, F., Steiner, J., 1996, in preparation.Google Scholar
Ferland, G.J., 1993, U. of Kentucky Dept. of Physics and Astronomy Internal Report.Google Scholar
Groenewegen, M.A.T., De Jong, T., 1994, Astronomy & Astrophysics, 282, 127.Google Scholar