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Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622
Context. Understanding of clouds is instrumental in interpreting current and future spectroscopic observations of exoplanets. Modeling clouds consistently is... 
Planetary atmospheres | Particle size | Nucleation | Clouds | Atmospheric models | Coagulation | Condensation | Optimization | Dependence | Cloud formation | Cloud thickness | Grain size | Spectroscopy | Parameters | Computer simulation | Extrasolar planets | Spectra | Sedimentation | Extrasolar giant planets | Thickness | Organic chemistry | Jupiter | Atmosphere | Particle transport | Astrochemistry | Transport | Computing time
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 11/2019, Volume 885, Issue 1, p. 79
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2014, Volume 572, pp. A72 - 31
Journal Article
ISSN 0035-8711, 2018
We present nested-grid, high-resolution hydrodynamic simulations of gas and particle dynamics in the vicinity of Mars- to Earth-mass planetary embryos. The... 
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 10/2017, Volume 606
Context. The Kepler mission has provided a large sample to statistically analyze the orbital properties of the super-Earth planet population. We hypothesize... 
Planets | Computer simulation | Extrasolar planets | Planet formation | Migration | Dispersal | Cavity expansion | Orbital resonances (celestial mechanics) | Configurations | Magnetospheres | Dispersion | Magnetic properties
Journal Article
Astronomy and Astrophysics - A&A, ISSN 0004-6361, 09/2014, Volume 572, p. A72
Context. Circumstellar disks are known to contain a significant mass in dust ranging from micron to centimeter size. Meteorites are evidence that individual... 
Solar and Stellar Astrophysics | Astrophysics | Earth and Planetary Astrophysics | Sciences of the Universe | Physics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 447, Issue 4, p. 3512
  Following Paper I we investigate the properties of atmospheres that form around small protoplanets embedded in a protoplanetary disc by conducting... 
Fluid mechanics | Astrophysics | Simulation | Extrasolar planets | Accretion disks | Star & galaxy formation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 447, Issue 4, pp. 3512 - 3512
Following Paper I we investigate the properties of atmospheres that form around small protoplanets embedded in a protoplanetary disc by conducting... 
Discs | Planets | Atmospheres | Protoplanets | Simulation | Replenishment | Disks | Atmospherics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 446, Issue 1, pp. 1026 - 1026
In the core accretion paradigm of planet formation, gas giants only form a massive atmosphere after their progenitors exceeded a threshold mass: the critical... 
Discs | Theorems | Rock | Planets | Atmospheres | Planet formation | Disks | Circulation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2015, Volume 446, Issue 1, p. 1026
  In the core accretion paradigm of planet formation, gas giants only form a massive atmosphere after their progenitors exceeded a threshold mass: the critical... 
Planets | Aeronomy | Atmosphere | Evolution | Star & galaxy formation
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2018, Volume 615
Turbulence plays a key role in the transport of pebble-sized particles. It also affects the ability of pebbles to be accreted by protoplanets because it stirs... 
Turbulence | Accretion | Turbulent flow | Computer simulation | Equations of motion | Turbulent diffusion | Inclination | Eddy diffusion | Particle inertia | Planets | Protoplanets | Settling | Deposition
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 07/2018, Volume 615
Context. Coagulation theory predicts that micron-sized dust grains grow into pebbles, which drift inward towards the star when they reach sizes of mm−cm. When... 
Circular orbits | Stokes number | Accretion | Computer simulation | Coagulation | Planetary mass | Planetary orbits | Embryos | Velocity | Jupiter | Eccentric orbits | Planet formation | Efficiency | Planetary evolution | Dependence | Drift | Computational efficiency | Orbital resonances (celestial mechanics) | Deposition | Planetary systems
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 02/2019, Volume 622, p. A121
Context. Understanding of clouds is instrumental in interpreting current and future spectroscopic observations of exoplanets. Modeling clouds consistently is... 
Planets and satellites: atmospheres | Methods: numerical | Planets and satellites: composition | planets and satellites: atmospheres | CONDENSATION CLOUDS | DUST | HOMOGENEOUS NUCLEATION | BROWN DWARFS | HAZE | ASTRONOMY & ASTROPHYSICS | planets and satellites: composition | OPACITIES | methods: numerical
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 07/2014, Volume 789, Issue 1, p. L18
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2014, Volume 441, Issue 3, p. 2380
  High levels of exozodiacal dust have been observed in the inner regions of a large fraction of main-sequence stars. Given the short lifetime of the observed... 
Extrasolar planets | Correlation analysis | Scattering | Star & galaxy formation
Journal Article
Journal Article
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