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The fraction of solar-type stars having stellar or massive nonstellar companions
Authors:Clifford Bettis  Jerry Bonnell  David Branch
Institution:Department of Physics and Astronomy, University of Oklahoma, Norman, Oklahoma 73019, USA
Abstract:The results of the survey for multiplicity by Abt and Levy are used to estimate the fraction of solar-type stars having close companions more massive than 0.01 solar masses. Current knowledge of the multiplicity characteristics of solar-type stars does not require that the fraction be nearly unity.
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