Non–adiabatic tidal oscillations induced by a planetary companion

Non–adiabatic tidal oscillations induced by a planetary companion

We calculate the dynamical tides raised by a close planetary companion on non–rotating stars of 1 M⊙ and 1.4 M⊙. Using the Henyey method, we solve the fully non–adiabatic equations throughout the star. The horizontal Lagrangian displacement is found to be 10 to 100 times larger than the equilibrium...

Полное описание

Библиографические подробности
Главные авторы:	Bunting, A, Papaloizou, J, Terquem, C
Формат:	Journal article
Язык:	English
Опубликовано:	Oxford University Press 2019

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