HT Cas
Image Credit: Mukai et al 1997, ApJ 475, 812.
The folded ASCA eclipse light curve 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.
This file was last modified on Friday, 09-Jul-1999 12:04:53 EDT
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