The central parsec of ngc 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region

HIGHLIGHTS

• who: GRAVITY Collaboration and colleagues from the der, CO, USA Research School of Astronomy and Astrophy tional University, Canberra, ACT, Austral Instituto de Astronomía, Universidad Nacional ApdoPostal, Ciudad de Méxixo, Department of Physics, Technical Universi have published the research: The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region, in the Journal: (JOURNAL) of April/20,/2019
• what: The new data the authors report here present a new look at this innermost region of NGC 3783. In Fig 8b the authors show . . .
  

   

  

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