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Interaction of a close-in extrasolar planet with the magnetic field of its host star
, 2013 Randy Olivier Laine
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Astronomy and Astrophysics, 2017
The surface rotations of some red giants are so fast that they must have been spun up by tidal interaction with a close companion, either another star, a brown dwarf, or a planet. We focus here on the case of red giants that are spun up by tidal interaction with a planet.
Christophe Lovis +2 more
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The surface rotations of some red giants are so fast that they must have been spun up by tidal interaction with a close companion, either another star, a brown dwarf, or a planet. We focus here on the case of red giants that are spun up by tidal interaction with a planet.
Christophe Lovis +2 more
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ON THE DIVERSITY OF MAGNETIC INTERACTIONS IN CLOSE-IN STAR-PLANET SYSTEMS [PDF]
Astrophysical Journal, 2014 18 pages, 11 figures, 4 tables, accepted for publication in The Astrophysical ...
Sean Matt, Antoine Strugarek
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2020
Among the numerous lessons learnt thanks to the CoRoT mission, it is now clear that stellar systems should be considered as a whole, i.e. including both the planets and their host star. While the communities interested in exo-planetary sciences and stellar physics were bound together by the same instrument, CoRoT, it soon appeared that they share a ...
LANZA, Antonino Francesco +2 more
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Among the numerous lessons learnt thanks to the CoRoT mission, it is now clear that stellar systems should be considered as a whole, i.e. including both the planets and their host star. While the communities interested in exo-planetary sciences and stellar physics were bound together by the same instrument, CoRoT, it soon appeared that they share a ...
LANZA, Antonino Francesco +2 more
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2019
In Chaps. 10 and 11, I surveyed the various ways in which a host star’s radiation and wind can erode an exoplanet’s atmosphere, change its chemistry, and thereby determine whether the exoplanet could be habitable. I now turn to the question of whether an exoplanet can change the properties of its host star, in particular, its rotation rate, UV and X ...
openaire +1 more source
In Chaps. 10 and 11, I surveyed the various ways in which a host star’s radiation and wind can erode an exoplanet’s atmosphere, change its chemistry, and thereby determine whether the exoplanet could be habitable. I now turn to the question of whether an exoplanet can change the properties of its host star, in particular, its rotation rate, UV and X ...
openaire +1 more source
Planet-star interactions with precise transit timing
Astronomy and Astrophysics, 2022Gracjan Maciejewski +2 more
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