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Ionization models of symbiotic stars

  • H. Nussbaumer
Part of the Astrophysics and Space Science Library book series (ASSL, volume 145)

Summary

A model of a symbiotic system is outlined. We present evidence that the main ionization mechanism responsible for the symbiotic nebula is radiative and not collisional. For calculating fractional ionization throughout the emission region we take either a blackbody source or an accreting system. If the ionizing radiation is due to accretion, the boundary layer between accreting star and disc provides the bulk of the ionizing photons. The possibility for distinguishing between different ionization sources are briefly discussed. C/N and O/N abundance ratios, calculated with the outlined ionization model places HM Sge, RS Oph, and T CrB among the novae and not among the symbiotic stars.

Keywords

Accretion Disc White Dwarf Stellar Wind Ionization Structure Planetary Nebula 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • H. Nussbaumer
    • 1
  1. 1.Institute of AstronomyETH ZentrumZürichSwitzerland

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