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

Author(s):
Amorim, A.; Bauböck, M.; Brandner, W.; Bolzer, M.; Clénet, Y.; Davies, R.; Zeeuw, P.T. de (0000-0003-4175-3474); 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.
Published
2021
Publication type
Article / Letter to editor
Galaxies: activeGalaxies: nucleiGalaxies: SeyfertQuasars: individual: NGC 3783Astrophysics - astrophysics of galaxiesAstrophysics - high energy astrophysical phenomena
Date issued
2021
Language
English
Is part of
Astronomy and Astrophysics (2021), Vol. 648, p. 1-24
hdl
1887/3273972
doi
10.1051/0004-6361/202040061
URL
https://ui.adsabs.harvard.edu/abs/2021A&A...648A.117G