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Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 4, pp. 4345 - 4353
With hydrodynamical simulations, we determine the conditions under which an initially coplanar planet-disc system that orbits a member of amisaligned binary star evolves to form a planet that undergoes Kozai-Lidov (KL... 
Hydrodynamics | Binaries: General | Accretion, accretion discs | Planets and satellites: Formation | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Giant stars | Simulation | Double stars | Planetology | Extrasolar planets | Accretion disks | Orbitals | Planets | Planet formation | Misalignment | Planetary evolution | Oscillations | Inclination | Physics - Earth and Planetary Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 1432-0746, 12/2016, Volume 596, p. A90
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 04/2018, Volume 612, p. A93
.... We aim to test whether stars harbouring hot Jupiters and stars with more distant gas-giant planets show any chemical peculiarity that could be related to different formation processes. Methods... 
Stars: abundances | Stars: late-type | Techniques: spectroscopic | Planetary systems | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Aluminum | Migration | Stars | Iron | Planetary mass | Orbits | Statistical methods | Planet formation | Titanium | Snow line | Silicon | Magnesium | Copper | Statistical analysis | Extrasolar planets | Abundance | Statistical tests | Zinc | Extrasolar giant planets | Organic chemistry | Jupiter | Planets | Metallicity | Gas giant planets | Chromium | Nickel | Chemical fingerprinting | Manganese
Journal Article