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This article has been cited by the following article(s):
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Hydrogen and helium shell burning during white dwarf accretion
CXO J004318.8+412016, a steady supersoft X-ray source in M 31
Marina Orio, G. J. M. Luna, R. Kotulla, et al. Monthly Notices of the Royal Astronomical Society 470(2) 2212 (2017) https://doi.org/10.1093/mnras/stx1355