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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 5.

Surface density and eccentricity evolution for the circumbinary disk. Here ed represents the mass-averaged particle eccentricity magnitude and is used as a statistical measure of orbital noncircularity. From top to bottom, the rows show the results for models with (eb = 0,  q = 1.92), (eb = 0.2,  q = 1.92), (eb = 0.4,  q = 1.92), (eb = 0,  q = 1.00), and (eb = 0,  q = 0.52), respectively (runs 5–9).

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