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We recalculated the maximum white dwarf mass in ultra-compact X-ray binaries   obtained in an earlier paper (Arbutina 2011), by taking the effects of   super-Eddington accretion rate on the stability of mass transfer into   account. It is found that, although the value formally remains the same   (under the assumed approximations), for white dwarf masses M2 >~0.1MCh mass   ratios are extremely low, implying that the result for Mmax is likely to have   little if any practical relevance

serbian astronomical journal/serbian astronomical journal

Maximum mass ratio of am CVn-type binary systems and maximum white dwarf mass in ultra-compact x-ray binaries (addendum - Serb. Astron. J. No. 183 (2011), 63)