Eccentric mass transfer via the new GeMT model accounts for the eccentric orbits of wide sdB+MS binaries as a direct consequence of mass-transfer physics.
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Updated ab initio tidal models predict Earth survives the Sun's giant phases, but outcomes depend strongly on AGB mass-loss rates, with L2 Pup observations as proxy indicating survival while low rates lead to engulfment.
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Eccentricity as a probe of mass-transfer physics. Eccentric mass transfer as a solution to the wide eccentric binary problem
Eccentric mass transfer via the new GeMT model accounts for the eccentric orbits of wide sdB+MS binaries as a direct consequence of mass-transfer physics.
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The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
Updated ab initio tidal models predict Earth survives the Sun's giant phases, but outcomes depend strongly on AGB mass-loss rates, with L2 Pup observations as proxy indicating survival while low rates lead to engulfment.