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Morphological and Kinematical Modelling of PNe and Nova Shells Using XSHAPE

Published online by Cambridge University Press:  26 May 2016

D. J. Harman ,
M. Bryce ,
T. J. O'Brien  and
J. Meaburn
D. J. Harman
Affiliation:
Jodrell Bank Observatory, Department of Physics and Astronomy, University of Manchester, Macclesfield, Cheshire, SK11 9DL
M. Bryce
Affiliation:
Jodrell Bank Observatory, Department of Physics and Astronomy, University of Manchester, Macclesfield, Cheshire, SK11 9DL
T. J. O'Brien
Affiliation:
Jodrell Bank Observatory, Department of Physics and Astronomy, University of Manchester, Macclesfield, Cheshire, SK11 9DL
J. Meaburn
Affiliation:
Jodrell Bank Observatory, Department of Physics and Astronomy, University of Manchester, Macclesfield, Cheshire, SK11 9DL

Abstract

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XSHAPE has been developed to aid the better understanding of the 3D morphologies and kinematics of PNe and novae, by producing models which closely predict the observed 2D images and long-slit spectra of these objects. Early successes include plausible simulations for the elliptical PN Sa 2-21 and the nova HR Del.

Type
Part VII: Nebular Morphology and Dynamics
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003 , pp. 531 - 532
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Meaburn, J., Blundell, B., Carling, R., Gregory, D. F., Keir, D., & Wynne, C. G. 1984, MNRAS, 210, 463 Google Scholar
Harman, D. J. 2001, , Google Scholar
Harman, D. J., Bryce, M., & Holloway, A. J. 2001, MNRAS, in prep Google Scholar
Harman, D. J., O'Brien, T. J., & Meaburn, J. 2001, MNRAS, in prep Google Scholar