Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
about
Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet ImagerAn abundant population of small irregular satellites around JupiterAn extrasolar planetary system with three Neptune-mass planetsOne or more bound planets per Milky Way star from microlensing observationsExoplanetary Atmospheres-Chemistry, Formation Conditions, and HabitabilityMetallicity of solar-type stars with debris discs and planetsBirth and fate of hot-Neptune planetsA massive planet to the young disc star HD 81040Debris disks as signposts of terrestrial planet formationMetallicity of M dwarfsThe HARPS search for southern extra-solar planets. V. A 14 Earth-masses planet orbiting HD 4308The metallicity signature of evolved stars with planetsStellar parameters and chemical abundances of 223 evolved stars with and without planetsFirst principles molecular dynamics study of filled ice hydrogen hydrate.How common are habitable planets?The formation of Uranus and Neptune in the Jupiter-Saturn region of the Solar System.Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes.Occurrence and core-envelope structure of 1-4× Earth-size planets around Sun-like starsA high C/O ratio and weak thermal inversion in the atmosphere of exoplanet WASP-12b.Disk evolution, element abundances and cloud properties of young gas giant planets.Detection of carbon monoxide and water absorption lines in an exoplanet atmosphere.Jupiter's decisive role in the inner Solar System's early evolution.Growing the gas-giant planets by the gradual accumulation of pebbles.Extra-solar planetary systems.Exploring the diversity of Jupiter-class planets.Planetary system formation in thermally evolving viscous protoplanetary discs.Infrared spectroscopy of exoplanets: observational constraints.Age of Jupiter inferred from the distinct genetics and formation times of meteorites.Possible climates on terrestrial exoplanets.Hot Jupiters from secular planet-planet interactions.Direct imaging of exoplanets.Migration-induced architectures of planetary systems.LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single offspring of stars that are rich in heavy elements.Surface growth kinematics via local curve evolution.Thermodynamic constrains for life based on non-aqueous polar solvents on free-floating planets.Detecting structure in a protostellar disk.Modeling the Jovian subnebula. I. Thermodynamic conditions and migration of proto-satellitesEnhanced collisional growth of a protoplanet that has an atmosphereOn uncertainty of Jupiter's core mass due to observational errorsSpectroscopic metallicities of Vega-like stars
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Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
description
im November 1996 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 1996
@uk
name
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
@en
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
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type
label
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
@en
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
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prefLabel
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
@en
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
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P2093
P356
P1433
P1476
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
@en
P2093
James B. Pollack
Morris Podolak
Olenka Hubickyj
Peter Bodenheimer
Yuval Greenzweig
P356
10.1006/ICAR.1996.0190
P577
1996-11-01T00:00:00Z