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BROWN DWARF BINARIES FROM DISINTEGRATING TRIPLE SYSTEMS

  • Authors: Bo Reipurth and Seppo Mikkola

2015 The Astronomical Journal 149 145.

  • Provider: AAS Journals

Caption: Figure 27.

Fraction of time that a companion spends at separations r larger than the semimajor axis a as a function of eccentricity. For orbits that are nearly circular, the fraction is as expected about 50%, but for an eccentricity of 1 it is 82%.

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