THE AM CVN SYSTEMS – THE FINAL STAGE OF BINARY WHITE DWARF EVOLUTION
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 e...
Main Authors: | J. -E. Solheim, M. R. Nasser |
---|---|
Format: | Article |
Language: | English |
Published: |
Odessa I. I. Mechnykov National University
2017-04-01
|
Series: | Odessa Astronomical Publications |
Online Access: | http://oap.onu.edu.ua/article/view/99498 |
Similar Items
-
AM CVn - finally solved? Results of XCOV4, March 1990
by: Solheim J.-E.
Published: (1993-09-01) -
The secondary star in AM CVn
by: Nymark T. K., et al.
Published: (1995-09-01) -
Maximum mass ratio of AM CVn-type binary systems and maximum white dwarf mass in ultra-compact X-ray binaries
by: Arbutina Bojan
Published: (2011-01-01) -
The AM CVn type stars: an overview
by: Solheim J.-E.
Published: (1995-09-01) -
A 3-D SPH model of helium accreation disks in the interacting binary white dwarf systems AM CVn and EC 15330-1403
by: Wood M. A., et al.
Published: (1995-09-01)