Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets
M. I. Jones, J. S. Jenkins, P. Rojo, C. Melo
Abstract
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M. I. Jones, J. S. Jenkins, P. Rojo, C. Melo
Abstract
Open-access reader
Context. To date, more than 30 planets have been discovered around giant stars, but only one of them has been found to be orbiting within 0.6 AU from the host star, in direct contrast to what is observed for FGK dwarfs. This result suggests that evolved stars destroy/engulf close-in planets during the red giant phase.
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Context. To date, more than 30 planets have been discovered around giant stars, but only one of them has been found to be orbiting within 0.6 AU from the host star, in direct contrast to what is observed for FGK dwarfs. This result suggests that evolved stars destroy/engulf close-in planets during the red giant phase.
Key concepts: Physics, Planet, Astrophysics, Stars, Red-giant branch, Star (game theory), RADIUS, Context (archaeology)