Tidal decay and stable Roche-lobe overflow of short-period gaseous exoplanets
نویسندگان
چکیده
منابع مشابه
Hot subdwarfs from the stable Roche lobe overflow channel
Context. Hot subdwarfs are core-helium-burning stars with extremely thin envelopes. We discuss the formation and evolution of hot subdwarfs formed through the stable Roche lobe overflow (RLOF) channel of intermediate-mass binaries, although their formation channels are various. Aims. In this study, we concentrate on the formation and evolution of hot subdwarfs binaries through the stable RLOF c...
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Many exoplanets have now been detected in orbits with ultra-short periods, very close to the Roche limit. Building upon our previous work, we study the possibility that mass loss through Roche lobe overflow (RLO) may affect the evolution of these planets, and could possibly transform a hot Jupiter into a lower-mass planet (hot Neptune or super-Earth). We focus here on systems in which the mass ...
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ژورنال
عنوان ژورنال: Celestial Mechanics and Dynamical Astronomy
سال: 2016
ISSN: 0923-2958,1572-9478
DOI: 10.1007/s10569-016-9704-1