Spectral optical monitoring of the double-peaked emission line AGN Arp 102B
Luka Č. Popović(Chinese Academy of Sciences), J. Torrealba(National Institute of Astrophysics, Optics and Electronics), A. N. Burenkov(Special Astrophysical Observatory), D. Ilić(Universität Hamburg), W. Kollatschny(University of Göttingen), J. León-Tavares(Aalto University), V. Patiño-Álvarez(National Institute of Astrophysics, Optics and Electronics), Andjelka B. Kovačević(Chinese Academy of Sciences), N. G. Bochkarev(Astronomical Institute of the Slovak Academy of Sciences), J. R. Valdés(National Institute of Astrophysics, Optics and Electronics), A. I. Shapovalova(Irkutsk State University), V. Chavushyan(National Institute of Astrophysics, Optics and Electronics)
Cited by 42
Related Papers
3D radiative transfer modelling of the dusty tori around active galactic nuclei as a clumpy two-phase medium
|Monthly Notices of the Royal Astronomical Society|2012|406
The MUSE <i>Hubble </i>Ultra Deep Field Survey
|Astronomy and Astrophysics|2017|343
Steps toward determination of the size and structure of the broad-line region in active galatic nuclei. 8: an intensive HST, IUE, and ground-based study of NGC 5548
|The Astrophysical Journal Supplement Series|1995|254
The MUSE 3D view of the<i>Hubble</i>Deep Field South
|Astronomy and Astrophysics|2015|227
Simultaneous<i>Planck</i>,<i>Swift</i>, and<i>Fermi</i>observations of X-ray and<i>γ</i>-ray selected blazars
|Astronomy and Astrophysics|2012|226