At the LBV star P Cyg the ARAS group is observing at present a more or less evenly descend to a historical minimum of the Halpha EW (see attached Fig.). This phenomenon is accompanied of a decreasing of the time distance between the separated minima.
We (the world-wide located P Cyg observers) are trying to continue this monitoring as long as it is possible, in order to follow the observed phenomenon.
Any comments are welcome!!