The AM CVn Systems - the Final Stage of Binary White Dwarf Evolution

Details The AM CVn Systems - the Final Stage of Binary White Dwarf Evolution The AM CVn Systems - the Final Stage of Binary White Dwarf Evolution

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001oap....14...98s&link_type=abstract

Odessa Astronomical Publications, 14, 98-105

Astronomy and Astrophysics

Astronomy

Stars: Binary: Cataclysmic, Interacting, Helium Cataclysmic, Stars: Individual: Am Cvn, Hp Lib, V803 Cen, Cr Boo, Cp Eri, Gp Com, Ce 315, Rx J1914+24

Scientific paper

The last decade has shown a surge in research on the Interacting Binary White Dwarf s (IBWDs), 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.

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