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- W2121489689 abstract "We report on the discovery of a 25.5-min superhump period for the suspected helium dwarf nova system KL Draconis in a high state. The presence of superhumps combined with the previously observed helium spectrum and large-amplitude photometric variations confirm that KL Dra is an AM CVn system similar to CR Bootis, V803 Cen and CP Eridani. We also find a low-state photometric period at 25.0 min that we suggest may be the orbital period. With this assumption, we estimate q=0.075, M1=0.76 M⊙ and M2=0.057 M⊙." @default.
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- W2121489689 date "2002-07-01" @default.
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- W2121489689 title "Superhumps in the helium dwarf nova KL Draconis" @default.
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- W2121489689 doi "https://doi.org/10.1046/j.1365-8711.2002.05484.x" @default.
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