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    • Disks around weak-line T Tauri stars 

      Gras-Velázquez, Àgueda (Trinity College (Dublin, Ireland). School of Physics, 2006)
      The formation of low -mass (M ~ 1 M⊙) stars has generally been divided into four stages before reaching the main sequence: Class 0 (cloud of gas and dust) -> Class I (embedded star with disk in envelope) -> Class II (visible ...