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Cited article:

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Can near-to-mid Infrared Spectral Energy Distribution Quantitatively Trace Protoplanetary Disk Evolution?

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Linking Circumstellar Disk Lifetimes to the Rotational Evolution of Low-mass Stars

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The Time Evolution of Md/Ṁ in Protoplanetary Disks as a Way to Disentangle between Viscosity and MHD Winds

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Forming Gas Giants around a Range of Protostellar M-dwarfs by Gas Disk Gravitational Instability

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