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Physical conditions in NGC 6543

Published online by Cambridge University Press:  25 May 2016

Nancy Jo Lame ,
J. Patrick Harrington  and
K. Borkowski
Nancy Jo Lame
Affiliation:
1University of Maryland, College Park
J. Patrick Harrington
Affiliation:
1University of Maryland, College Park
K. Borkowski
Affiliation:
2North Carolina State University

Extract

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We observed NGC 6543 (the Cat's Eye Nebula) with the HST WFPC2 camera in ten narrow-band filters covering a range of emission lines. These images are used to further look at the physical conditions in NGC 6543. We discuss the [O III] electron temperature, ionization state throughout the nebula, and the results of photoionization models of individual structures.

Type
IV. Envelopes
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 252 - 253
Copyright
Copyright © Kluwer 1997 

References

de Koter, A., Heap, S.R., Hubeny, I., & Lanz, T. 1996, preprint.Google Scholar
Ferland, G. J. 1993, University of Kentucky Department of Physics and Astronomy Internal Report.Google Scholar
Kingdon, J.B., & Ferland, G.J. 1995, ApJ, 450,691.Google Scholar
Kingsburgh, R. L., López, J. A., & Peimbert, M. 1996, in: Cosmic Abundances, eds. Holt, S. and Sonneborn, G., ASP Conf. Ser. 99, p. 350.Google Scholar