R. Staubert, S. Schandl, J. Wilms
Institut für Astronomie und Astrophysik, Astronomie, Universität Tübingen, Waldhäuser Str. 64, D-72076 Tübingen, Germany
To appear in: Proc. of the 5th Compton Symposium, ed. M. McConnell
Abstract. In Her X-1 the history of the 35 day turn-ons is strongly correlated with the histories of the 1.24 s pulsations and the X-ray ux. We suggest a common origin for these correlated variations, namely a variable mass transfer rate.Key words: -
Paper (55k gzip'ed Postscript including figures)
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