Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-11T02:22:09.004Z Has data issue: false hasContentIssue false
  • English
  • Français

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.
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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