ASCA light curve of HT Cas
This folded ASCA eclipse light curve is of the nonmagnetic cataclysmic variable HT Cas. The upper panel shows the data and the best-fit model, the lower panel the residuals. The short transitions to and out of the eclipse indicate that the X-ray emission region is not much larger than the white dwarf primary.
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Last modified: Thursday, 26-Jun-2003 13:48:44 EDT
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