Tidally induced non-adiabatic stellar oscillations: how planets make stars wobble
<p>We calculate the dynamical tides raised by a close planetary companion on non-rotating stars of 1 M<sub>⊙</sub> and 1:4 M<sub>⊙</sub>. Using the Henyey method, we solve the fully non-adiabatic equations throughout the star, both for the case of frozen convection and...
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| Médium: | Diplomová práce |
| Jazyk: | English |
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2020
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