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Brown dwarf companion with a period of 4.6 yr interacting with the hot Jupiter CoRoT-20b

Rey, J. (author)
Université de Genève,University of Geneva
Bouchy, F. (author)
Université de Genève,University of Geneva
Stalport, M. (author)
Université de Genève,University of Geneva
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Deleuil, M. (author)
Laboratoire d'Astrophysique de Marseille
Hebrard, G. (author)
Institut d 'Astrophysique de Paris,Observatoire de Haute-Provence
Almenara, J. M. (author)
Université de Genève,University of Geneva
Alonso, R. (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Barros, S.C.C. (author)
Universidade do Porto,University of Porto
Bonomo, A. S. (author)
Istituto nazionale di astrofisica (INAF)
Cazalet, G. (author)
Laboratoire d'Astrophysique de Marseille
Delisle, J. B. (author)
Université de Genève,University of Geneva
Diaz, R. F. (author)
Universidad de Buenos Aires
Fridlund, Malcolm, 1952 (author)
Chalmers tekniska högskola,Chalmers University of Technology,Universiteit Leiden (UL),Leiden University (UL)
Guenther, E. W. (author)
Instituto de Astrofísica de Canarias,Thüringer Landessternwarte Tautenburg
Guillot, T. (author)
Observatoire de la Cote d'Azur
Montagnier, G. (author)
Observatoire de Haute-Provence,Institut d 'Astrophysique de Paris
Moutou, C. (author)
Canada France Hawaii Telescope Corporation
Lovis, C. (author)
Université de Genève,University of Geneva
Queloz, D. (author)
University Of Cambridge
Santerne, A. (author)
Laboratoire d'Astrophysique de Marseille
Udry, S. (author)
Université de Genève,University of Geneva
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 (creator_code:org_t)
2018-11-13
2018
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 619
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • We report the discovery of an additional substellar companion in the CoRoT-20 system based on six years of HARPS and SOPHIE radial velocity follow-up. CoRoT-20 c has a minimum mass of 17 ± 1 MJup and orbits the host star in 4.59 ± 0.05 yr, with an orbital eccentricity of 0.60 ± 0.03. This is the first identified system with an eccentric hot Jupiter and an eccentric massive companion. The discovery of the latter might be an indication of the migration mechanism of the hot Jupiter, via the Lidov-Kozai effect. We explore the parameter space to determine which configurations would trigger this type of interactions.

Subject headings

TEKNIK OCH TEKNOLOGIER  -- Maskinteknik -- Rymd- och flygteknik (hsv//swe)
ENGINEERING AND TECHNOLOGY  -- Mechanical Engineering -- Aerospace Engineering (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
MEDICIN OCH HÄLSOVETENSKAP  -- Medicinsk bioteknologi -- Biomedicinsk laboratorievetenskap/teknologi (hsv//swe)
MEDICAL AND HEALTH SCIENCES  -- Medical Biotechnology -- Biomedical Laboratory Science/Technology (hsv//eng)

Keyword

Planetary systems
Brown dwarfs
Stars: Low-mass
Planets and satellites: Dynamical evolution and stability
Techniques: Radial velocities
Stars: Individual: CoRoT-20

Publication and Content Type

art (subject category)
ref (subject category)

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