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...

Szczegółowa specyfikacja

Opis bibliograficzny
Główni autorzy:	Bunting, A, Papaloizou, J, Terquem, C
Format:	Journal article
Język:	English
Wydane:	Oxford University Press 2019

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