(Q53966788)

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Modeling the Jovian subnebula. I. Thermodynamic conditions and migration of proto-satellites

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Modeling the Jovian subnebula. I. Thermodynamic conditions and migration of proto-satellites (English)

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1

Y. Alibert

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Willy Benz

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3

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W. Benz

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O. Mousis

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2

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language of work or name

English

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publication date

12 August 2005

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published in

Astronomy and Astrophysics

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volume

439

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issue

3

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page(s)

1205–1213

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cites work

Formation of the Galilean Satellites: Conditions of Accretion

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stated in

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reference URL

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21 January 2018

Distributions of CO2 and SO2 on the surface of Callisto

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21 January 2018

Carbon dioxide on Ganymede

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reference URL

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retrieved

21 January 2018

Formation of the regular satellites of giant planets in an extended gaseous nebula I: subnebula model and accretion of satellites

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reference URL

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retrieved

21 January 2018

Shock Compression of Deuterium and the Interiors of Jupiter and Saturn

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21 January 2018

Implications from Galileo Observations on the Interior Structure and Chemistry of the Galilean Satellites

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21 January 2018

Oceans in the icy Galilean satellites of Jupiter?

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reference URL

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retrieved

21 January 2018

Planetary science. Jupiter and its moons

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reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20052841

retrieved

21 January 2018

Three‐dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet Migration

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retrieved

21 January 2018

Outward migration of extrasolar planets to large orbital radii

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reference URL

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retrieved

21 January 2018

Formation of the Giant Planets by Concurrent Accretion of Solids and Gas

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stated in

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reference URL

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retrieved

21 January 2018

Orbital migration of the planetary companion of 51 Pegasi to its present location

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stated in

Crossref

reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20052841

retrieved

21 January 2018

Identifiers

DOI

10.1051/0004-6361:20052841

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1 reference

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ResearchGate publication ID

248851695

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(Q53966788)

Modeling the Jovian subnebula. I. Thermodynamic conditions and migration of proto-satellites

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