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Doppler tomography for investigation of binary central stars in planetary nebulae: computer modeling

Published online by Cambridge University Press:  15 December 2006

O. I. Sharova
O. I. Sharova
Affiliation:
Radiophysical Research Institute, Nizhny Novgorod, 603950, Russia email: shol@nirfi.sci-nnov.ru.
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Abstract

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The radio astronomical approach is applied to 2D and 3D Doppler tomography for close binary central stars in planetary nebulae. It is more effective than the traditional one.

Keywords

binaries: closeplanetary nebulae: generaltechniques: image processing
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S234: Planetary Nebulae in our Galaxy and Beyond , April 2006 , pp. 507 - 508
Copyright
© 2006 International Astronomical Union