THE AM CVN SYSTEMS – THE FINAL STAGE OF BINARY WHITE DWARF EVOLUTION
DOI:
https://doi.org/10.18524/1810-4215.2001.14.99498Ключові слова:
Stars, binary, cataclysmic, interacting, helium cataclysmic, stars, individual, AM CVn, HP Lib, V803 Cen, CR Boo, CP Eri, GP Com, CE 315, RX J1914 24Анотація
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.Посилання
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