つくば宇宙理論コロキウム

第47

Protoplanetary disk evolution: fragmentation and dust ring formation

松⽊場 亮喜

京都大学


要旨
We study the metallicity dependence of the disk fragmentation using 2D hydrodynamics simulations. We perform long-term simulations up to 0.1 Myr with a wide metallicity range of $10^{-5}Z_{\odot}

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