@misc{SandinSteffenJacobetal.2011,
  author    = {Sandin, Christer and Steffen, Matthias and Jacob, Ralf and Sch{\"o}nberner, Detlef and R{\"u}hling, Ute and Hamann, Wolf-Rainer and Todt, Helge Tobias},
  title     = {The role of heat conduction to the formation of [WC]-type planetary nebulae},
  series = {Proceedings of the International Astronomical Union},
  journal   = {Proceedings of the International Astronomical Union},
  number    = {582},
  issn      = {1866-8372},
  doi       = {10.25932/publishup-41370},
  url       = {http://nbn-resolving.de/urn:nbn:de:kobv:517-opus4-413702},
  pages     = {494 -- 495},
  year      = {2011},
  abstract  = {X-ray observations of young Planetary Nebul{\ae} (PNe) have revealed diffuse emission in extended regions around both H-rich and H-deficient central stars. In order to also repro-duce physical properties of H-deficient objects, we have, at first, extended our time-dependent radiation-hydrodynamic models with heat conduction for such conditions. Here we present some of the important physical concepts, which determine how and when a hot wind-blown bubble forms. In this study we have had to consider the, largely unknown, evolution of the CSPN, the slow (AGB) wind, the fast hot-CSPN wind, and the chemical composition. The main conclusion of our work is that heat conduction is needed to explain X-ray properties of wind-blown bubbles also in H-deficient objects.},
  language  = {en}
}