THE AM CVN SYSTEMS – THE FINAL STAGE OF BINARY WHITE DWARF EVOLUTION
In: Odessa Astronomical Publications, Jg. 14 (2017), Heft 0, S. 98-105
Online
academicJournal
Zugriff:
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.
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THE AM CVN SYSTEMS – THE FINAL STAGE OF BINARY WHITE DWARF EVOLUTION
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Autor/in / Beteiligte Person: | J. -E. Solheim ; Nasser, M. R. |
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Zeitschrift: | Odessa Astronomical Publications, Jg. 14 (2017), Heft 0, S. 98-105 |
Veröffentlichung: | Odessa I. I. Mechnykov National University, 2017 |
Medientyp: | academicJournal |
ISSN: | 1810-4215 (print) |
DOI: | 10.18524/1810-4215.2001.14.99498 |
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