
About 2/3 of all hot subdwarfs are in binaries with either long-periods with FGK-type companions or short-periods with brown dwarf or M-dwarf, or white dwarf companions. With current surveys, the number of known systems increased significantly. We obtain mass and period distributions of both components, and the population membership using their kinematics.
Session 3: Binaries, Triple Systems, & Interactions, Session 3: Binaries, Triple Systems, & Interactions
Session 3: Binaries, Triple Systems, & Interactions, Session 3: Binaries, Triple Systems, & Interactions
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