arXiv · astro-ph/9612030
The X-ray off-state of the supersoft source CAL 83 and its interpretation
Abstract
We consider simultaneous optical data obtained during the recent X-ray turn-off of CAL83. Combining the optical behaviour with the observed X-ray decay time, we show that a model of cessation of steady nuclear burning is viable if the white dwarf is massive. Our model provides a natural explanation for the subsequent return of the supersoft X-ray emission.
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C. Alcock et al. 1996-12-03. The X-ray off-state of the supersoft source CAL 83 and its interpretation. https://doi.org/10.1093/mnras%2F286.2.483
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