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Circumbinary Disk Formation through AGB Star Winds

  • Authors: Shunquan Huang, 顺权 黄, Rebecca G. Martin

Shunquan Huang et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 6.

Snapshots of the projected density at t = 2681.22 yr (350 binary orbital periods) for simulations employing different EoSs. The left and right columns show the locally isothermal (run 5) and binary isothermal (run 10) models, respectively. The bottom row presents zoomed-in views of the companion region. The blue circle indicates the companion’s accretion radius (0.4 au).

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