A highly non-keplerian protoplanetary disc – spiral structure in the gas disc of cq tau

HIGHLIGHTS

• who: Wölfer L. et al. from the Max-Planck-Institut für extraterrestrische Physik, Gießenbachstr1, Garching bei München, Germany Departamento de Astronomía, Universidad de Chile, Camino El Observatorio, Las Condes, Santiago, Chile have published the article: A highly non-Keplerian protoplanetary disc - Spiral structure in the gas disc of CQ Tau, in the Journal: (JOURNAL)
• what: The authors aim to analyse the gas brightness temperature and kinematics of the transitional disc around the intermediatemass star CQ Tau to resolve and characterise substructure in the gas caused by possible perturbers. The paper . . .
  

   

  

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