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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 1.

Specific energy ein for the injected particles as a function of the angle ϕ1, measured relative to the direction toward the companion, for various binary mass ratios q and specific energy ratio η. The angle ϕ1 = 0° corresponds to the point on the stellar surface facing the companion.

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