Oscillations in solar-type stars tidally induced by orbiting planets
We examine the effect of dynamical tides raised by a companion on a solar-type star. In these binaries, gravity or g mode oscillations are excited by the companion in the radiative region beneath the convective envelope of the star. They become evanescent in the convection zone. This is of particula...
| Hlavní autoři: | , , , |
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| Médium: | Journal article |
| Vydáno: |
1997
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