Left panels
Top: View onto the close, eclipsing, post common-envelope binary system AA Dor,
that consists of a sdOB-type primary star and an unseen low-mass companion,
from the top and from the
side (as seen from Earth, i = 89.21 degrees).
Bottom: Normalized synthetic lightcurve
Right panels
Phase-dependent spectral variation of the He II 4686Å line profile.
Our UVES spectra (bottom, smoothed by a Gaussian of 0.05Å FWHM) is compared with the synthetic spectrum (top).
A smaller version (1.9 MB) of this animation can be downloaded here.
Top: View onto the binary system AA Dor from the side (as seen from Earth, i = 89.21 degrees).
The illuminated part of the cool companion is shown.
Bottom: Phase-dependent synthetic spectrum around Hβ