Probing the heart of an active galactic nucleus: NGC 1068

被引:0
|
作者
Tecza, M
Thatte, N
Maiolino, R
机构
[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
[2] Osserv Astrofis Arcetri, I-50125 Florence, Italy
关键词
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results from integral field spectroscopy of the narrow line region of NGC 1068, carried out with the MPE 3D near infrared imaging spectrometer. A map and velocity field of the [Fe II] fine structure line at 1.64mum is presented. The kinematics of the [Fe II] emission, which arises in partially ionized zones, shows red shifted emission in the north eastern cone of the NLR, and blue shifted emission in the south west, reversed relative to high ionization species such as [Si VI] or [0 111]. We propose a model geometry of the narrow line region which is consistent with existing data and explains the observed [Fe II] kinematics.
引用
收藏
页码:216 / 219
页数:4
相关论文
共 50 条
  • [1] Molecular emission in the active galactic nucleus of NGC 1068
    Galliano, E
    Alloin, D
    INTERPLAY AMONG BLACK HOLES, STARS AND ISM IN GALACTIC NUCLEI, 2004, (222): : 259 - 262
  • [2] OUTFLOWING DIFFUSE GAS IN THE ACTIVE GALACTIC NUCLEUS OF NGC 1068
    Geballe, T. R.
    Mason, R. E.
    Oka, T.
    ASTROPHYSICAL JOURNAL, 2015, 812 (01):
  • [3] FOOTPRINTS OF AN ACTIVE GALACTIC NUCLEUS - THE NUCLEAR ZONE OF NGC-1068
    BALICK, B
    HECKMAN, T
    ASTRONOMICAL JOURNAL, 1985, 90 (02): : 197 - 203
  • [4] Why does NGC 1068 have a more powerful active galactic nucleus than NGC 4258?
    Murayama, T
    Taniguchi, Y
    PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, 1997, 49 (04) : L13 - L18
  • [5] Why does NGC 1068 have a more powerful active galactic nucleus than NGC 4258?
    Astronomical Institute, Tohoku University, Aoba, Sendai
    980-77, Japan
    Publ. Astron. Soc. Jpn., 1600, 4 (L13-L18):
  • [6] 0.6 resolution images at 11 and 20 μm of the active galactic nucleus in NGC 1068
    Alloin, D
    Pantin, E
    Lagage, PO
    Granato, GL
    ASTRONOMY & ASTROPHYSICS, 2000, 363 (03) : 926 - 932
  • [7] Galactic outflow driven by the active nucleus and the origin of the gamma-ray emission in NGC 1068
    Lamastra, A.
    Fiore, F.
    Guetta, D.
    Antonelli, L. A.
    Colafrancesco, S.
    Menci, N.
    Puccetti, S.
    Stamerra, A.
    Zappacosta, L.
    ASTRONOMY & ASTROPHYSICS, 2016, 596
  • [8] Gas and stellar dynamics in NGC 1068: probing the galactic gravitational potential
    Emsellem, E
    Fathi, K
    Wozniak, H
    Ferruit, P
    Mundell, CG
    Schinnerer, E
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 365 (02) : 367 - 384
  • [9] MULTIDIRECTIONAL VIEWS OF THE ACTIVE NUCLEUS OF NGC-1068
    MILLER, JS
    GOODRICH, RW
    MATHEWS, WG
    ASTROPHYSICAL JOURNAL, 1991, 378 (01): : 47 - 64
  • [10] The central dusty torus in the active nucleus of NGC 1068
    W. Jaffe
    K. Meisenheimer
    H. J. A. Röttgering
    Ch. Leinert
    A. Richichi
    O. Chesneau
    D. Fraix-Burnet
    A. Glazenborg-Kluttig
    G.-L. Granato
    U. Graser
    B. Heijligers
    R. Köhler
    F. Malbet
    G. K. Miley
    F. Paresce
    J.-W. Pel
    G. Perrin
    F. Przygodda
    M. Schoeller
    H. Sol
    L. B. F. M. Waters
    G. Weigelt
    J. Woillez
    P. T. de Zeeuw
    Nature, 2004, 429 : 47 - 49