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相关论文: The Nuclear Outflow in NGC 2110

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The analysis of the optical spectra of PMN J0948+0022 showed significant variations in the spectral lines that, when combined with the Fermi $\gamma$-ray light curve and radio observations reported by other authors, were interpreted as the…

高能天体物理现象 · 物理学 2025-11-25 B. Dalla Barba , L. Foschini , M. Berton , A. Lähteenmäki , M. Tornikoski , E. Sani , L. Crepaldi , E. Congiu , G. Venturi , W. J. Hon , A. Vietri

We present ultraviolet emission-line maps of the narrow-line region (NLR) of NGC 1068. The maps span 115--318 nm, the biconical ionization cone, several posited jet/ISM interactions, and the compact knots whose optical spectra we reported…

天体物理学 · 物理学 2008-11-26 Brent Groves , Gerald Cecil , Pierre Ferruit , Michael Dopita

We present a case study of HE 0040-1105, an unobscured radio-quiet AGN at a high accretion rate (Eddington ratio = 0.19+/-0.04). This particular AGN hosts an ionized gas outflow with the largest spatial offset from its nucleus compared to…

We have discovered an extremely broad, double-peaked H-alpha emission line in the polarized flux spectrum of NGC 2110, establishing that this well-studied Seyfert 2 galaxy contains a disk-like hidden broad-line region (BLR). Several…

天体物理学 · 物理学 2009-11-13 Edward C. Moran , Aaron J. Barth , Michael Eracleous , Laura E. Kay

We present the first interferometric HCN(J = 3-2) and HCO+(J = 3-2) maps in the circumnuclear region of NGC 1097, obtained with the Submillimeter Array. The goal is to study the characteristics of the dense gas associated with the starburst…

宇宙学与河外天体物理 · 物理学 2015-06-03 Pei-Ying Hsieh , Paul T. P. Ho , Kotaro Kohno , Chorng-Yuan Hwang , Satoki Matsushita

The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxygen, and nitrogen, as well as the CO(4-3) molecular line. The…

星系天体物理 · 物理学 2017-03-01 F. P. Israel , R. Guesten , R. Meijerink , M. A. Requena-Torres , J. Stutzki

Accretion and ejection of matter in active galactic nuclei (AGN) are tightly connected phenomena and represent fundamental mechanisms regulating the growth of the central supermassive black hole and the evolution of the host galaxy.…

We present near-infrared and optical emission-line and stellar kinematics of the Seyfert 2 galaxy Mrk 573 using the Near-Infrared Field Spectrograph (NIFS) at Gemini North and Dual Imaging Spectrograph (DIS) at Apache Point Observatory,…

AGN activity is known to drive fast outflows of gas. We report the discovery of fast outflows of neutral gas with velocities over 1000 km/s in a number of radio galaxies. In the best studied object, 3C~293, the kinematical properties of the…

天体物理学 · 物理学 2009-11-10 T. A. Oosterloo , R. Morganti , B. H. C. Emonts , C. N. Tadhunter

We analyzed near-infrared data of the nearby galaxy IC5063 taken with the Very Large Telescope SINFONI instrument. IC5063 is an elliptical galaxy that has a radio jet nearly aligned with the major axis of a gas disk in its center. The data…

星系天体物理 · 物理学 2015-12-23 K. M. Dasyra , A. C. Bostrom , F. Combes , N. Vlahakis

Archival Hubble Space Telescope (HST) observations of the Seyfert 1 nucleus of NGC 3227 obtained with the Space Telescope Imaging Spectrograph (STIS) are re-examined in order to constrain a viable photoionization model for the broad-line…

星系天体物理 · 物理学 2020-10-07 Nick Devereux

AGN-driven outflows are believed to play an important role in regulating the growth of galaxies mostly via negative feedback. However, their effects on their hosts are far from clear, especially for low and moderate luminosity Seyferts. To…

Large-scale outflows driven by AGNs are an important element of galaxy evolution. Detailed analysis of their properties allows us to probe the activity history of the galactic nucleus and, potentially, other properties of the host galaxy. A…

星系天体物理 · 物理学 2025-10-17 Kastytis Zubovas , Matas Tartėnas

High-resolution observations in the near infrared show star clusters around the active galactic nucleus (AGN) of the Seyfert 1 NGC2110, along with a 90 x 35 pc bar of shocked gas material around its nucleus. These are seen for the first…

星系天体物理 · 物理学 2015-06-18 Mark Durré , Jeremy Mould

Although the properties of the narrow-line region (NLR) of active galactic nuclei(AGN) have been deeply studied by many authors in the past three decades, many questions are still open. The main goal of this work is to explore the NLR of…

宇宙学与河外天体物理 · 物理学 2015-06-11 L. Vaona , S. Ciroi , F. Di Mille , V. Cracco , G. La Mura , P. Rafanelli

Massive outflows are known to exist, in the form of extended emission-line regions (EELRs), around about one-third of powerful FR II radio sources. We investigate the origin of these EELRs by studying the emission-line regions around…

宇宙学与河外天体物理 · 物理学 2015-06-16 Hsin-Yi Shih , Alan Stockton , Lisa Kewley

Extended narrow-line regions (ENLRs) and extended emission-line regions (EELRs) have been the focus of integral field spectroscopy aiming at the inner kiloparsecs of nearby Seyfert galaxies as well as the larger environment of high redshift…

宇宙学与河外天体物理 · 物理学 2011-07-05 J. Scharwaechter , M. A. Dopita , J. Zuther , S. Fischer , S. Komossa , A. Eckart

We present an analytical model for the hydrodynamic outflow from the disk of a starburst galaxy. The model is used to calculate the cosmic ray propagation and the radio intensity distribution in the nuclear starbust region of NGC 253. We…

天体物理学 · 物理学 2016-08-30 V. N. Zirakashvili , H. J. Voelk

We present near-infrared VLT ISAAC imaging and spectroscopy of the peculiar Virgo galaxy NGC 4438, whose nucleus has been classified as a LINER. The data are supplemented by mid-infrared imaging, and compared to previous WFPC2 HST broadband…

星系天体物理 · 物理学 2015-05-14 Sebastian Perez , Simon Casassus , Juan R. Cortes , J. D. P. Kenney

We present near-infrared ($H$- and $K$-band) integral-field observations of the inner $\sim$700pc of the active spiral galaxy NGC613, obtained with SINFONI on the Very Large Telescope. We use emission-line ratios to determine the dominant…

星系天体物理 · 物理学 2015-06-17 J. Falcón-Barroso , C. Ramos Almeida , T. Böker , E. Schinnerer , J. H. Knapen , A. Lançon , S. Ryder