Structure and Transport in the Solar Neb
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A. Drouart; B. Dubrulle; D. Gautier; F. Robert
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Article
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1999
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Elsevier Science
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English
โ 494 KB
A simplified analytical model of an evolutionary nebula is used to generate temperature-density radial profiles following the procedure elaborated by Dubrulle (Icarus 106, 59, 1993). Each nebula disk is characterized by its initial mass M D , its initial radius R D , and the coefficient of turbulent