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EMPIRICAL TIDAL DISSIPATION IN EXOPLANET HOSTS FROM TIDAL SPIN–UP
Stars with hot Jupiters tend to be rotating faster than other stars of the same age and mass. This trend has been attributed to tidal interactions between the star and planet. A constraint on the dissipation parameter [Formula: see text] follows from the assumption that tides have managed to spin up...
Gorde:
| Argitaratua izan da: | Astron J |
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| Egile Nagusiak: | , , , |
| Formatua: | Artigo |
| Hizkuntza: | Inglês |
| Argitaratua: |
2018
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| Gaiak: | |
| Sarrera elektronikoa: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6510550/ https://ncbi.nlm.nih.gov/pubmed/31080254 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/1538-3881/aaaf71 |
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