Orbital Circularization of Hot and Cool Kepler Eclipsing Binaries
The rate of tidal circularization is predicted to be faster for relatively cool stars with convective outer layers, compared to hotter stars with radiative outer layers. Observing this effect is challenging because it requires large and well-characterized samples that include both hot and cool stars...
| Κύριοι συγγραφείς: | , , |
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| Άλλοι συγγραφείς: | |
| Μορφή: | Άρθρο |
| Γλώσσα: | en_US |
| Έκδοση: |
IOP Publishing
2016
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| Διαθέσιμο Online: | http://hdl.handle.net/1721.1/104931 https://orcid.org/0000-0002-4265-047X |