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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 2.

Specific entropy s (top row), H (bottom row, solid lines), and He (bottom row, dashed lines) TAMS profiles for nonrotating single stars (red), accretors (orange), and “engineered” models of the same total mass as the post-RLOF mass of the accretors. The overlapping gray bands emphasize the CEB region, X c(1H) + 0.01 < X(1H) < X surf(1H) − 0.01, with X c and X surf the central and surface value of the hydrogen mass fraction. The CEB size of the engineered models increases from blue to yellow.

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