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Deprojection of Planetary Nebula Images

Published online by Cambridge University Press:  07 August 2017

K. Volk  and
D. A. Leahy
K. Volk
Affiliation:
Department of Physics and Astronomy, University of Calgary, 2500, University Drive N.W., Calgary, Alberta, Canada T2N 1N4
D. A. Leahy
Affiliation:
Department of Physics and Astronomy, University of Calgary, 2500, University Drive N.W., Calgary, Alberta, Canada T2N 1N4

Extract

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We present first results of the deprojection of some optical and radio images of planetary nebulae using an iterative technique based on the Lucy method, as discussed in Leahy (1991). This approach allows a greater range of possible geometries to be investigated and is less sensitive to the effects of noise compared with the direct matrix-inversion method which can be used for the spherical case. We assume that the emissivity function can be represented as

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 372
Copyright
Copyright © Kluwer 1993 

References

Leahy, D. A. 1991, A&A, 247, 584 Google Scholar