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Rejuvenated Accretors Have Less Bound Envelopes: Impact of Roche Lobe Overflow on Subsequent Common Envelope Events

  • Authors: M. Renzo, E. Zapartas, S. Justham, K. Breivik, M. Lau, R. Farmer, M. Cantiello, B. D. Metzger

M. Renzo et al 2023 The Astrophysical Journal Letters 942 .

  • Provider: AAS Journals

Caption: Figure 6.

The structure of the CEB at the end of the main sequence impacts the envelope binding energy profile throughout the remaining evolution. Dashed lines show the gravitational contribution only; while solid lines include the contribution of the internal energy. The red lines show a 30 M , nonrotating, Z = 0.0019 model compared to “engineered” models of the same mass (see Figure 5, increasing CEB size from blue to yellow), but artificially imposed profile at TAMS (other colors; see text). The top (bottom) axis indicates mass coordinate (radius). We compare the models when they first reach 500 R .

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