Oblique filament collisions lead to gravitational collapse of the compressed cloud when post-collision |gravitational energy| exceeds kinetic plus thermal plus magnetic energies, with lower angles and lower velocities favoring hub-filament formation.
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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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Evolution of compressed clouds formed by filament coalescence. I. Oblique collisions
Oblique filament collisions lead to gravitational collapse of the compressed cloud when post-collision |gravitational energy| exceeds kinetic plus thermal plus magnetic energies, with lower angles and lower velocities favoring hub-filament formation.
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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.