The Best Guess: Testing new and old formalisms for the common envelope against observations
Riley Thai, Amanda Karakas, Zara Osborn, Robert Izzard, Ryosuke Hirai, Alex Kemp, Simon Campbell
astro-ph.SR
Submitted: 2026-08-19
Updated: 2026-08-20
Comments: 29 pages, 14 (8+6) figures. Submitted to ApJ, all comments welcome
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess
- Searching for GEMS: Discovery of the Nearby Post-Common-Envelope Binary System TIC-460388167
- On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution
- Common envelopes in massive stars III. The obstructive role of radiation transport in envelope ejection
- The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
- Dust Formation in Common Envelope Binary Interactions -- III. Lightcurves
- Reconstructing the evolution of double helium white dwarfs: envelope loss without spiral-in
- Weakened inspirals -- I: High mass ratio common envelope interactions in RGB stars
- The Origin and Evolution of Multiple Star Systems
- A global view of post-interaction white dwarf-main sequence binaries
- Stability Criteria for Mass Transfer in Binary Stellar Evolution
- Common Envelope Evolution Redux
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