Journal article
Oscillations in solar-type stars tidally induced by orbiting planets
- Abstract:
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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 particular interest in connection with the newly discovered planets, some of which are found to orbit around solar-type stars with a period comparable to that of the high order g modes of the star. One such...
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Bibliographic Details
- Publication date:
- 1997-11-19
- Source identifiers:
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363722
Item Description
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- Pubs id:
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pubs:363722
- UUID:
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uuid:d5b4ed5b-6c9a-4e5a-bdb7-d71012dac76e
- Local pid:
- pubs:363722
- Deposit date:
- 2013-11-16
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- Copyright date:
- 1997
- Notes:
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5 pages with 1 Postscript figure, LaTeX. To be published in the
Proceedings of the IXemes Rencontres de Blois "Planetary Systems: The Long
View" (Blois, June 1997), Editions Frontieres
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