Turbulence within a single core leads to multiple dense clumps. These clumps independently collapse to form stars that orbit each other. Gravitational instabilities in a massive accretion disk cause the formation of a similar, secondary disk within the first ,resulting in two stars that orbit each other.
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Stars are not always single ,most of them are combined, having 2 od more star systems ,for instance Alpha Centuari is a system of 3 stars
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