Binary stars within multipolar planetary nebulae
1 : Nicolaus Copernicus University
* : Corresponding author
We undertook a 3D-model analysis of several planetary nebulae which show quite complicated geometries - quadrupolar or even more. The first IFU spectra from an ongoing observing project with ARGUS instrument at ESO were obtained for M 3-38. We present here the spatial and kinematical structure of this nebula and discuss it in the context of indirect evidences of central binary system like: high-velocity extended bipolar outflows, compact dusty inner torus, complex of recombination emission lines near 465 nm.
| Subject : | : | Posters |
| Topics | : | Shaping |
| PDF version | : |  PDF version |
