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Morpho-kinematic modeling of planetary nebulae with SHAPE

Published online by Cambridge University Press:  15 December 2006

Wolfgang Steffen  and
José Alberto López
Wolfgang Steffen
Affiliation:
Instituto de Astronomía, UNAM, Ensenada, México email: [email protected]
José Alberto López
Affiliation:
Instituto de Astronomía, UNAM, Ensenada, México email: [email protected]
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Abstract

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We present a powerful new tool to disentangle the 3-D geometry and kinematic structure of gaseous nebulae. The method consists of combining commercially available digital animation software to simulate the 3-D structure and expansion pattern of the nebula with a dedicated, purpose built rendering software and graphical user interface that produce the final images and long slit spectra which are compared to the real data.

Keywords

stars: windsoutflowsplanetary nebulae: generalmethods: miscellaneous
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 517 - 518
Copyright
© 2006 International Astronomical Union