About: Rapid growth of gas-giant cores by pebble accretion

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scientific article published in Astronomy and Astrophysics

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована в липні 2012 (uk) im Juli 2012 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astronomy and Astrophysics (fr) scientific article published in Astronomy and Astrophysics (en)
publication date	wds:Q56169105-92738000-E75A-4B7A-B6A8-EB771CCE0855
publication date	2012-07-20 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56169105-9709BC00-8B19-434C-8CE0-336CC477CC8A
language of work or name	English
cites work	wds:Q56169105-094189D2-D31E-465C-ABD3-43E80EF73A1F wds:Q56169105-1A20E589-31B2-44A3-A0E3-5CC30AADC07F wds:Q56169105-1B1D5AA4-AED9-4474-A1DC-814548D0C3A2 wds:Q56169105-3DE9D05F-73D3-4513-B391-ED2BADFE3A34 wds:Q56169105-43E33020-AF60-4542-8BFF-EB221DB015FB wds:Q56169105-4C10089B-3358-4E04-9120-5AB8567FF53C wds:Q56169105-5DCAC05C-AAE9-445C-AD85-7A8C4134C452 wds:Q56169105-67951116-899E-4B85-9CED-5158F99FA134 wds:Q56169105-93EA2C8F-8541-4326-BFB4-86193F7A5C45 wds:Q56169105-96DE8AC2-FAFF-4521-A726-A62098B71646 wds:Q56169105-99DC1AAD-BBA8-4255-88D7-01C1BABE0310 wds:Q56169105-9E92498A-F9D2-432E-AA4E-940999D1B492 wds:Q56169105-A8C7B4D8-D629-4328-97D9-8A2A2E0DD421 wds:Q56169105-AB42C0EB-4215-4132-BC64-A02F3F302EB2 wds:Q56169105-C04A7256-0CB3-4214-ADA1-57C9E8414A51 wds:Q56169105-D8FBC891-3D34-4E89-8B2F-83E4949B303F wds:Q56169105-DF86F40E-5C56-42B0-AE5B-177C85FB1599 wds:Q56169105-F106EA1A-8E9F-4AA3-ABA6-AE57C4F68635 wds:Q56169105-F390E870-C2B9-4653-BF67-E4664213A326 wds:Q56169105-F95261DA-C67C-4774-9E3A-0342D13D2FC7 wds:Q56169105-FC0D6722-49CD-4D97-AB71-0033FCECED08
cites work	The Planet‐Metallicity Correlation Spectroscopic [Fe/H] for 98 extra-solar planet-host stars A low mass for Mars from Jupiter's early gas-driven migration Optical images of an exosolar planet 25 light-years from Earth A giant planet imaged in the disk of the young star beta Pictoris Images of a fourth planet orbiting HR 8799. Formation of the Giant Planets by Concurrent Accretion of Solids and Gas Solar System Abundances and Condensation Temperatures of the Elements A powerful local shear instability in weakly magnetized disks. I - Linear analysis. II - Nonlinear evolution Rapid planetesimal formation in turbulent circumstellar disks Disk Frequencies and Lifetimes in Young Clusters Structure of the Solar Nebula, Growth and Decay of Magnetic Fields and Effects of Magnetic and Turbulent Viscosities on the Nebula Atmospheres of Protoplanetary Cores: Critical Mass for Nucleated Instability Dust flow in gas disks in the presence of embedded planets Toward Planetesimals in the Disk around TW Hydrae: 3.5 Centimeter Dust Emission The last gasp of gas giant planet formation: a Spitzer study of the 5 Myr old cluster NGC 2362 Infrared non-detection of Fomalhaut b: implications for the planet interpretation LkCa 15: A YOUNG EXOPLANET CAUGHT AT FORMATION? Three‐dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration Adding particle collisions to the formation of asteroids and Kuiper belt objects via streaming instabilities Accretion Disks around Young Stars: Lifetimes, Disk Locking, and Variability
author name string	wds:Q56169105-3A16E200-F579-46B6-A1D6-12983C5A0C68
author name string	M. Lambrechts
rdfs:label	Rapid growth of gas-giant cores by pebble accretion (en) Rapid growth of gas-giant cores by pebble accretion (nl)
skos:prefLabel	Rapid growth of gas-giant cores by pebble accretion (en) Rapid growth of gas-giant cores by pebble accretion (nl)
name	Rapid growth of gas-giant cores by pebble accretion (en) Rapid growth of gas-giant cores by pebble accretion (nl)
author	wds:Q56169105-B890DB46-8143-4B08-93A4-BB588F691998
author	Anders Johansen
title	wds:Q56169105-FCF64055-D4F0-413E-B27D-73D273886EC5
title	Rapid growth of gas-giant cores by pebble accretion (en)
page(s)	wds:Q56169105-AB5EB484-9D28-4F44-9155-C74D61414EB4
page(s)	32–32
instance of	wds:Q56169105-472A0631-9495-4A98-BBCF-3C2FAD2EAC68
instance of	scholarly article
published in	wds:Q56169105-AAECD77D-3F32-4120-B7CE-9652FB986F9F
published in	Astronomy and Astrophysics
volume	wds:Q56169105-B8E4C402-BEF8-4A18-B17A-DD2ABBC6BBB4
volume	544
DOI	wds:Q56169105-A663323C-8BFD-4591-8C0F-65511CBD872C
DOI	http://dx.doi.org/10.1051/0004-6361/201219127
DOI	10.1051/0004-6361/201219127
ResearchGate publication ID	wds:Q56169105-1584A299-660B-416A-9239-C0772E529C96
ResearchGate publication ID	224951911
arXiv ID	wds:Q56169105-CB34BE3F-159B-4494-A910-47548F56C93B
arXiv ID	1205.3030
ADS bibcode	wds:Q56169105-C656E551-9821-4414-B318-47130D0E7DFD
ADS bibcode	2012A&A...544A..32L
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56169105
is cites work of	Discovery and spectroscopy of the young jovian planet 51 Eri b with the Gemini Planet Imager First light of the VLT planet finder SPHERE Growing the gas-giant planets by the gradual accumulation of pebbles The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits. II. Survey description, results, and performances A library of near-infrared integral field spectra of young M–L dwarfs Is there an exoplanet in the Solar system? Carbon-rich planet formation in a solar composition disk Isotopic evidence for primordial molecular cloud material in metal-rich carbonaceous chondrites Age of Jupiter inferred from the distinct genetics and formation times of meteorites Isotopic evolution of the protoplanetary disk and the building blocks of Earth and the Moon. Challenges in planet formation Formation of Venus, Earth and Mars: Constrained by Isotopes The nature of the TRAPPIST-1 exoplanets Collision velocity of dust grains in self-gravitating protoplanetary discs Growing the terrestrial planets from the gradual accumulation of submeter-sized objects The VLT/NaCo large program to probe the occurrence of exoplanets and brown dwarfs at wide orbits. IV. Gravitational instability rarely forms wide, giant planets Hot super-Earths and giant planet cores from different migration histories

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