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Insights on CAIs Thermal History from Turbulent Transport Simulations of Micron-Sized Precursors in the Early Solar Nebula

E. Taillifet 1 K. Baillié S. Charnoz J. Aléon 2
1 CSNSM AS
CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
2 CSNSM - Centre de Sciences Nucléaires et de Sciences de la Matière
Abstract : Using numerical simulations we showed that turbulent transport in a thermally zoned protoplanetary disk might be at the origin of CAIs complexity and diversity.
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http://hal.in2p3.fr/in2p3-00945946
Contributor : Christine Hadrossek <>
Submitted on : Thursday, February 13, 2014 - 11:39:06 AM
Last modification on : Sunday, December 6, 2020 - 3:08:02 AM

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E. Taillifet, K. Baillié, S. Charnoz, J. Aléon. Insights on CAIs Thermal History from Turbulent Transport Simulations of Micron-Sized Precursors in the Early Solar Nebula. 44th Lunar and Planetary Science Conference, 2013, The Woodlands, United States. pp.2007. ⟨in2p3-00945946⟩

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