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DYNAMICAL ACCRETION OF PRIMORDIAL ATMOSPHERES AROUND PLANETS WITH MASSES BETWEEN 0.1 AND 5M⊕IN THE HABITABLE ZONE

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Hydrostatic, isothermal planetary models from the point of view of dynamical systems: “Determination of explicit formulas for the point of critical mass”

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CRITICAL CORE MASSES FOR GAS GIANT FORMATION WITH GRAIN-FREE ENVELOPES

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