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ASCA Guest Observer Facility

HT Cas

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
Curator: Michael Arida (SP Sys); arida@milkyway.gsfc.nasa.gov
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This file was last modified on Friday, 09-Jul-1999 12:04:53 EDT

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