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Proceedings of Accretion Processes in Cosmic Sources — PoS(APCS2016)
SDSS J090221.35+381941.9 is an Cataclysmic Variable AM CVn system that has three most likely evolutionary tracks as defined by the donor type -the hydrogen star channel, the white dwarf channel, and the helium star channel. To break the degeneracy, we numerically model this system three different ways, one for each channel, keeping the mass transfer rate, orbital period, and secondary-to-primary mass ratio constant. Because the white dwarf channel produced a shorter Stage A positive superhumpdoi:10.22323/1.288.0019 fatcat:o6rghmoqqnbfjn4kaa5wmsbz2u