Cepheids. It gets worse!
|Title||Cepheids. It gets worse!|
|Author(s)||Robert S Fritzius|
Subsequently retitled "Non-pulsating Cepheid Variables"
Vladimir Sekerin felt he could explain Cepheid variables using Ritz's c+v effects. This page is a continuation of that idea.
The cyclic color changes of Cepheid variables appear to be consistent with Ritz c+v information arrival time modulation. This modulation is such that during a brightness peak there is a time-wise compression of the observed spectrum, which produces higher observed frequencies. If there were to be evenly spaced time markers impressed on the luminous flux (at the source) we would see that their time-wise spacing decreases during the bright phase, reaching minimum separation at the brightness peak. During the lower intensity "trough" of the light curve the time markers would be stretching further apart, reaching maximum separation at minimum intensity. As the arrival time "clock" varies in speed, the stellar spectrum changes in color (Hottest at peak, coolest at trough.) Here, we are considering a bright star with a dim (mostly unseen) companion...