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Accretion Processes in CV AM CVn SDSS J090221.35+381941.9
2018
Proceedings of Accretion Processes in Cosmic Sources — PoS(APCS2016)
unpublished
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 superhump
doi:10.22323/1.288.0019
fatcat:o6rghmoqqnbfjn4kaa5wmsbz2u