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Showing 1 to 1 of 1 for “"Class 0/I"”.

  1. Streaming Instabilities in Class 0/I Disks

    … so that we need to shift our focus to young Class 0/I disks to study the initial conditions for planet formation. To investigate this, we use global models of disk formation and evolution run with the non-ideal magnetohydrodynamic version of RAMSES, an adaptive mesh refinement code, with a …

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