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Deprojection of Planetary Nebulae

Published online by Cambridge University Press:  12 April 2016

Z.W. Zhang  and
W.H. Ip
Z.W. Zhang
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan, Email: m889002@astro.ncu.edu.tw
W.H. Ip
Affiliation:
Institute of Astronomy, National Central University, Chung-Li 32054, Taiwan, Email: m889002@astro.ncu.edu.tw

Abstract

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Useful information can be obtained by deprojection of the two-dimensional images of extended objects such as planetary nebulae or supernova remnants. Three-dimensional distributions (assumed to be axially symmetric) of emissivity, electron number density and temperature might be derived from the deprojected structures. As a test, we follow the iterative algorithm of Leahy & Volk (1994) to project the images of several PNe taken at different wavelengths. This method can also be applied to the images of supernova remnants and galaxy clusters.

Type
VII. Science With Small Telescopes
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 337 - 338
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

Aaquist, O.B.,& Kwok, S. 1996, APJ, 426, 813 Google Scholar
Leahy, L.A., & Volk, K. 1994, A&A, 282, 561 Google Scholar
Volk, k., & Leahy, L.A. 1993, AJ, 106, 1954 Google Scholar