
The contact binary system has been classified in five different types according to their physical properties. We suggest that extremely small mass ratio contact binary systems(q<0.2) could be classified as a new type of contact binaries in addition to the classification. According to the Svechnikov & Kuznetsova (1990)'s catalogue, the spectral types of primary components of newly classified contact binaries are distributed at A type, and also the distribution of their various physical characteristics is laid at the center region dividing the early-type contact binaries from late-type contact binaries.
classification, Astronomy, contact binary, QB1-991, small mass ratio contact bianry
classification, Astronomy, contact binary, QB1-991, small mass ratio contact bianry
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