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Chimie 3D de l’effondrement des cœurs denses - formation des disques protoplanétaires

Chimie 3D de l’effondrement des cœurs denses - formation des disques protoplanétaires. RAMSES Teyssier 2002 Fromang et al. 2006 Commerçon et al. 2011. NAUTILUS Hersant et al. 2009 Hincelin et al. 2011. Effondrement 3D (RMHD). Chimie gaz-grain. t=4.10 4 ans. T(K). 100. Chimie 3D. 300.

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Chimie 3D de l’effondrement des cœurs denses - formation des disques protoplanétaires

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  1. Chimie 3D de l’effondrement des cœurs denses - formation des disques protoplanétaires RAMSES Teyssier 2002Fromang et al. 2006Commerçon et al. 2011 NAUTILUS Hersant et al. 2009Hincelin et al. 2011 Effondrement 3D (RMHD) Chimie gaz-grain t=4.104ans T(K) 100 Chimie 3D 300 50 z(UA) 100 y(UA) 0 -50 30 -100 log n(cm-3) 100 13 y(UA) 50 12 y(UA) 0 x(UA) CO(gaz)/H 11 -50 10 -100 -100 -50 0 50 100 x(UA) Hincelin U., Commerçon B., Wakelam V., Hersant F., Guilloteau S., Aikawa Y. en préparation

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