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

  • R. E. Carlos Reyes (a1) (a2), J. E. Steiner (a1) and F. Elizalde (a2)

Extract

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.

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Copyright

References

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

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