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    • A disk of dust and molecular gas around a high-mass protostar 

      Patel, Nimesh A.; Curiel, Salvador; Tirupati, Tirupati Kumaran; Zhang, Qizhou; Hunter, Todd R.; Ho, Paul T. P.; Torrelles, José M.; Moran, James M.; Gómez, José F.; Anglada, Guillem (Springer Nature, 2005)
      The processes leading to the birth of low-mass stars such as our Sun have been well studied1, but the formation of high-mass (over eight times the Sun's mass, Mcircle dot) stars remains poorly understood2. Recent studies ...