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Haro 5-2: A New Pre-main-sequence Quadruple Stellar System

  • Authors: Bo Reipurth, C. Briceño, T. R. Geballe, C. Baranec, S. Mikkola, A. M. Cody, M. S. Connelley, C. Flores, B. A. Skiff, J. D. Armstrong, N. M. Law, R. Riddle

Bo Reipurth et al 2024 The Astronomical Journal 168 .

  • Provider: AAS Journals

Caption: Figure 10.

Left: example of chaotic transformation of a nonhierarchical system of four single stars into a temporary 2+2 quadruple (black/red + blue/green), which subsequently breaks up into a binary (black/red) and two single stars (blue and green). Right: example of a nonhierarchical configuration of two primordial binaries (2 and 3) that bind to form a stable 2+2 quadruple system, as an interloper flies by and carries away the excess energy. The formation of a quadruple system is far simpler when the binaries have formed prior to their interaction. Both simulations show the dynamical interactions of point sources without any gas.

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