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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 10.

Core mass remaining at the time when the triple systems have their last close triple encounter and the binary becomes bound, resulting in either a bound stable (red) or bound unstable (green) system or a disrupted system (gray). As the figure illustrates, stable triple systems are formed only in the presence of a cloud core. The few stable systems that are indicated as having been formed with near-zero gas mass are misclassified by the stability criterion, they are unstable and will eventually disrupt.

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