no code implementations • 16 Dec 2020 • P. Severgnini, V. Braito, C. Cicone, P. Saracco, C. Vignali, R. Serafinelli, R. Della Ceca, M. Dotti, F. Cusano, D. Paris, G. Pruto, A. Zaino, L. Ballo, M. Landoni
We found that most of the prominent optical emission lines are characterized by a double-peaked profile, mainly produced by AGN photoionization.
Astrophysics of Galaxies
