Odessa Astronomical Publications (Apr 2017)

THE AM CVN SYSTEMS – THE FINAL STAGE OF BINARY WHITE DWARF EVOLUTION

  • J. -E. Solheim,
  • M. R. Nasser

DOI
https://doi.org/10.18524/1810-4215.2001.14.99498
Journal volume & issue
Vol. 14, no. 0
pp. 98 – 105

Abstract

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The last decade has shown a surge in research on the Interacting Binary White Dwarf s (IB-WDs), or Helium CVs, also called AM CVn systems. We have witnessed long photometric campaigns, time resolved spectroscopy, UV and X-ray observations, and modelling of disc structure, disc atmosphere and their evolution. Recently several new members of the AM CVn family have been added, and a new subclass - double degenerate polars has been identified. A review of the research on AM CVn systems during the last decade is given, and some problems to be solved in the future are presented.