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Showing astro-ph.EPShow all
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astro-ph.EP2019★ 7 cited
The Rate of Planet-star Coalescences Due to Tides and Stellar Evolution
Alexander V. Popkov, Sergei B. Popov
Orbits of close-in planets can shrink significantly due to dissipation of tidal energy in a host star. This process can result in star-planet coalescence within the Galactic lifeti…
astro-ph.EP2015★ 53 cited
Imaging Jupiter's radiation belts down to 127 MHz with LOFAR
J. N. Girard, P. Zarka, C. Tasse +71
Context. Observing Jupiter's synchrotron emission from the Earth remains today the sole method to scrutinize the distribution and dynamical behavior of the ultra energetic electron…
astro-ph.EP2011★ 23 cited
Close encounters of a rotating star with planets in parabolic orbits of varying inclination and the formation of Hot Jupiters
P. B. Ivanov, J. C. B. Papaloizou
(abbreviated) We extend the theory of close encounters of a planet on a parabolic orbit with a star to include the effects of tides induced on the central rotating star. Orbits wit…