EE Cephei 2014 Eclipse Campaign
EE Cephei is a binary system composed by a Be star and some body that eclipses it each 5.5 years. It is the 2nd system of its kind, being epsilon Aurigae the other one.
My modest collaboration with the Alpy 600 :
A colleague of mine, David Boyd made a more intensive coverage of the eclipse. His results are published here:
http://adsabs.harvard.edu/abs/2014arXiv1412.5127B
I joined our results in one sheet.:
It is interesting to note how the Halpha line strengthens during the eclipse.