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Related papers: Modelling the ENLR in NGC1068

200 papers

We use the full broad-band XMM-Newton EPIC data to examine the X-ray spectrum of the nearby Seyfert 2 galaxy NGC 1068, previously shown to be complex with the X-ray continuum being a sum of components reflected/scattered from cold (neutral)…

Astrophysics · Physics 2009-11-11 K. Pounds , S. Vaughan

Despite being thought to play an important role in galaxy evolution, the true impact of outflows driven by active galactic nuclei (AGN) on their host galaxies is unclear. In part, this may be because electron densities of outflowing gas are…

Astrophysics of Galaxies · Physics 2023-06-28 Luke R. Holden , Clive N. Tadhunter

With the incorporation of high-J molecular lines, we aim to constrain the physical conditions of the dense gas in the central region of the Seyfert 2 galaxy NGC 1068 and to determine signatures of the AGN or the starburst contribution. We…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 J. P. Perez-Beaupuits , M. Spaans , F. F. S. van der Tak , S. Aalto , S. Garcia-Burillo , A. Fuente , A. Usero

We present a detailed study of the complex ionization structure in a small (~250 pc) extended narrow line region (ENLR) cloud near Centaurus A using the Multi Unit Spectroscopic Explorer. This cloud is located in the so-called outer…

Astrophysics of Galaxies · Physics 2016-05-04 F. Santoro , J. B. R. Oonk , R. Morganti , T. A. Oosterloo , C. Tadhunter

We analyze a XRISM/Resolve observation of NGC1068, focusing on the Fe K$\alpha$ and Fe K$\beta$ fluorescent lines and on the Fe XXV and Fe XXVI emission complexes. Line centroid energies, intrinsic widths, flux ratios, and constraints on…

The first complete far-infrared spectrum (43-197um) of the Seyfert 2 galaxy NGC 1068 as observed with the LWS onboard ISO is reported. In addition to the expected ionic fine structure emission lines, the OH rotational lines at 79, 119 and…

The latest observations of line and continuum spectra emitted from the extended narrow line region (ENLR) of the Seyfert 2 galaxy NGC 7212 are analysed using models accounting for photoionization from the active nucleus and shocks. The…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 M. Contini , V. Cracco , S. Ciroi , G. La Mura

(Abridged) We present a detailed analysis of a large sample of 31 low-redshift, mostly radio-quiet type 1 QSOs observed with integral field spectroscopy to study their extended emission-line regions (EELRs). We focus on the ionisation state…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-11 B. Husemann , L. Wisotzki , S. F. Sánchez , K. Jahnke

We present an unprecedented view on the morphology and kinematics of the extended narrow-line region (ENLR) and molecular gas around the prototypical hyper-luminous quasar 3C273 ($L\sim10^{47}$ erg/s at z=0.158) based on VLT-MUSE optical 3D…

Astrophysics of Galaxies · Physics 2019-07-17 B. Husemann , V. N. Bennert , K. Jahnke , T. A. Davis , J. -H. Woo , J. Scharwächter , A. Schulze , M. Gaspari , M. Zwaan

We have made the first VLBI synthesis images of the H2O maser emission associated with the central engine of the Seyfert galaxy NGC 1068. Emission extends about +/-300 km/s from the systemic velocity. Images with submilliarcsecond angular…

Astrophysics · Physics 2009-10-28 L. J. Greenhill , C. R. Gwinn , R. Antonucci , R. Barvainis

We present dynamical models based on a study of high-resolution long-slit spectra of the narrow-line region (NLR) in NGC 1068 obtained with the Space Telescope Imaging Spectrograph (STIS) aboard The Hubble Space Telescope (HST). The…

Astrophysics · Physics 2008-11-26 V. Das , D. M. Crenshaw , S. B. Kraemer

Active galactic nuclei (AGN) are characterized by similar broad emission lines properties at all luminosities ($10^{39}$-$10^{47}$ erg s$^{-1}$). What produces this similarity over a vast range of $10^8$ in luminosity? Photoionization is…

Cosmology and Nongalactic Astrophysics · Physics 2014-02-04 Alexei Baskin , Ari Laor , Jonathan Stern

Preliminary analysis of the X-ray spectrum of NGC 1068 obtained by the RGS spectrometer on board XMM-Newton is presented. A physically consistent model is developed in order to quantitatively describe the reprocessing of the central AGN…

We have mapped the extended narrow line region (ENLR) of NGC 3393 on scales of $r\lesssim4^{\prime\prime}$ ($\sim1\,$kpc) from the nucleus using emission line images of H$\alpha\,\lambda6563$, [O III]$\lambda5007$, and [S…

We aim to determine the properties of the central region of NGC 1052 using X-ray and radio data. NGC 1052 (z=0.005) has been investigated for decades in different energy bands and shows radio lobes and a low luminosity active galactic…

Astrophysics of Galaxies · Physics 2020-07-01 S. Falocco , J. Larsson , S. Nandi

We present models for the mid- and far- infrared emission from the Narrow Line Region (NLR) of Active Galactic Nuclei (AGN). Using the MAPPINGS III code we explore the effect of typical NLR parameters on the spectral characteristics of the…

Astrophysics · Physics 2009-11-11 Brent Groves , Michael Dopita , Ralph Sutherland

Outflows of ionized gas driven by active galactic nuclei (AGN) may significantly impact the evolution of their host galaxies. However, determining the energetics of these outflows is difficult with spatially unresolved observations that are…

We present a spatially resolved analysis of ionized gas at the nuclear region of the nearby galaxy NGC 1068. While NGC 1068 has been known to have gas outflows driven by its active galactic nucleus (AGN), more complex kinematical signatures…

Astrophysics of Galaxies · Physics 2021-02-24 Jaejin Shin , Jong-Hak Woo , Minjin Kim , Junfeng Wang

We present spatially resolved Chandra HETGS observations of the Seyfert 2 galaxy NGC 1068. X-ray imaging and high resolution spectroscopy are used to test the Seyfert unification theory. Fe K-alpha emission is concentrated in the nuclear…

Astrophysics · Physics 2009-11-07 P. M. Ogle , T. Brookings , C. R. Canizares , J. C. Lee , H. L. Marshall

We present Gemini/GNIRS spectroscopy of the Seyfert 2 galaxy NGC 4388, with simultaneous coverage from 0.85 - 2.5 $\mu$m. Several spatially-extended emission lines are detected for the first time, both in the obscured and unobscured portion…