Recombination energy is unlikely to drive steady transonic stellar winds from gravitationally bound gas without prior unbinding or radiative losses, but can accelerate pre-existing outflows to high mass-loss rates.
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The paper reviews departures from classical binary evolution theory for low- and intermediate-mass stars, focusing on eccentric orbits, mass exchange, tides, and eccentricity maintenance.
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Steady-state Stellar Winds Driven by Recombination
Recombination energy is unlikely to drive steady transonic stellar winds from gravitationally bound gas without prior unbinding or radiative losses, but can accelerate pre-existing outflows to high mass-loss rates.
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Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory
The paper reviews departures from classical binary evolution theory for low- and intermediate-mass stars, focusing on eccentric orbits, mass exchange, tides, and eccentricity maintenance.