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

Amorim, A.; Bauböck, M.; Brandner, W.; Bolzer, M.; Clénet, Y.; Davies, R.; de Zeeuw, P.T.; Dexter, J.; Drescher, A.; Eckart, A.; Eisenhauer, F.; Förster Schreiber, N.M.; Gao, F.; Garcia, P.J.V.; Genzel, R.; Gillessen, S.; Gratadour, D.; Hönig, S.; Kaltenbrunner, D.; Kishimoto, M.; Lacour, S.; Lutz, D.; Millour, F.; Netzer, H.; Ott, T.; Paumard, T.; Perraut, K.; Perrin, G.; Peterson, B.M.; Petrucci, P.O.; Pfuhl, O.; Prieto, M.A.; Rouan, D.; Sanchez-Bermudez, J.; Shangguan, J.; Shimizu, T.; Schartmann, M.; Stadler, J.; Sternberg, A.; Straub, O.; Straubmeier, C.; Sturm, E.; Tacconi, L.J.; Tristram, K.R.W.; Vermot, P.; von Fellenberg, S.; Waisberg, I.; Widmann, F.; Woillez, J.; Gravity Collaboration,

doi:10.1051/0004-6361/202040061

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

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Eckart, A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Amorim, A., Bauböck, M., Brandner, W., Bolzer, M., Clénet, Y., Davies, R., et al. (2021). The central parsec of NGC 3783: a rotating broad emission line region, asymmetric hot dust structure, and compact coronal line region. åp, 648: A117, pp. A117. doi:10.1051/0004-6361/202040061.

Cite as: https://hdl.handle.net/21.11116/0000-000A-73B0-D

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