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Created page with "[https://ui.adsabs.harvard.edu/abs/1996ApJS..105..181K/abstract D. G. Korycansky & J. C. B. Papaloizou (1996)]<br />''A Method for Calculations of Nonlinear Shear flow:<br />Application to Formation of Giant Planets in the Solar Nebula''<br />The Astrophysical Journal Supplements Series, Vol. 105, pp. 181 - 190" |
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[https://ui.adsabs.harvard.edu/abs/1996ApJS..105..181K/abstract D. G. Korycansky & J. C. B. Papaloizou (1996)]<br />''A Method for Calculations of Nonlinear Shear | [https://ui.adsabs.harvard.edu/abs/1996ApJS..105..181K/abstract D. G. Korycansky & J. C. B. Papaloizou (1996)]<br />''A Method for Calculations of Nonlinear Shear Flow:<br />Application to Formation of Giant Planets in the Solar Nebula''<br />The Astrophysical Journal Supplements Series, Vol. 105, pp. 181 - 190 | ||
Latest revision as of 22:03, 15 December 2023
D. G. Korycansky & J. C. B. Papaloizou (1996)
A Method for Calculations of Nonlinear Shear Flow:
Application to Formation of Giant Planets in the Solar Nebula
The Astrophysical Journal Supplements Series, Vol. 105, pp. 181 - 190