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Interacting Binary Stars as Progenitors for Interacting Supernovae

  • Authors: Sung-Han Tsai, Ke-Jung Chen, Keiichi Maeda, Po-Sheng Ou, Friedrich K. Röpke

Sung-Han Tsai et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

Binary interaction outcomes—noninteracting (red), Case C transfer (green), and Case B transfer (blue)—as a function of initial orbital separation and donor mass M1, assuming a fixed mass ratio q2 of 0.9. Hatched regions indicate models that undergo CEE. The boundary between interacting and noninteracting binaries shifts to larger separations with increasing total binary mass. A complex interaction landscape emerges at M1 ≲ 20, M and separations ≲3200 R, where multiple interaction channels coexist. CEE occurs predominantly for M1 ≲ 28 M and separations ≲2500 R.

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