Based on Robin's observation + and BAV homepage 1.5-1.7 Umag drop has just happened as in the past, light from the B component must be mostly out for now (yet to wait for making sure there is no more drop).
However, let me remind everyone, then we are now in a critical phase for the higher Balmer lines - as I've taken my lower UV region, Balmer is still there, suspectedly some parts still coming from the remaining internal part of an internal disk:
(Could not subtract M component yet for this region, need to wait till Alp Ori is up. Have Mu. Cep that is too far from perfect to subtract at this higher ratio.)
If our speculation is right and an internal disk exists with the high Balmer lines, we should see now how the above H14-H9 lines get "switched off" week by week!
As I've looked through the literature, no other known emission exist this region than 3806 [Cu II] (+ Balmer), so I expect the outstanding emission at H11 is really from H11.
Unfortunately, weather is poor here, but now I'd chose this region to follow next.
Cheers,
Peter