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相关论文: Helical structures in Seyfert galaxies

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We present our recent results about the extended narrow-line region (ENLR) of two nearby Seyfert 2 galaxies (IC 5063 and NGC 7212) obtained by modelling the observed line profiles and spectra with composite models (photoionization+shocks)…

Based on a new spectroscopic sample observed using the WHT, we examine the kinematic properties of the various emission line regions in narrow line Seyfert 1 galaxies (NLS1s) by modelling their profiles using multiple component fits. We…

天体物理学 · 物理学 2009-11-13 James R. Mullaney , Martin J. Ward

We have combined HST/FOS and ground-based spectra of the Seyfert 1 galaxy NGC 5548 to study the narrow emission lines over the 1200 -- 10,000 angstrom region. All of the spectra were obtained when the broad emission line and continuum…

天体物理学 · 物理学 2009-10-30 Steven B. Kraemer , D. Michael Crenshaw , Alexei V. Filippenko , Bradley M. Peterson

LINERs exist in the nuclei of a large fraction of luminous galaxies, but their connection with the AGN phenomenon has remained elusive. We present Hubble Space Telescope narrowband [O III]5007 and H-alpha+[N II] emission-line images of the…

天体物理学 · 物理学 2009-10-31 R. W. Pogge , D. Maoz , L. C. Ho , M. Eracleous

The narrow emission line spectra of active galactic nuclei are not accurately described by simple photoionization models of single clouds. Recent Hubble Space Telescope images of Seyfert 2 galaxies show that these objects are rich with…

天体物理学 · 物理学 2009-10-30 Jason W. Ferguson , Kirk T. Korista , Jack A. Baldwin , Gary J. Ferland

We have compared the morphological characteristics of the 891 galaxies in the Extended 12-micron Sample (E12GS), and assessed the effect of the 12-micron selection criterion on galaxy properties. The normal spirals in the E12GS have the…

天体物理学 · 物理学 2010-04-21 L. K. Hunt , M. A. Malkan

The recent detection of high-energy gamma rays from Narrow-Line Seyfert 1 Galaxies has confirmed that also this type of active galactic nuclei can generate powerful relativistic jets. I outline the evolution of the knowledge in this…

高能天体物理现象 · 物理学 2013-01-25 Luigi Foschini

We have compiled a list of 83 objects classified as Narrow-Line Seyfert 1 galaxies (NLS1s) or known to have a broad Balmer component narrower than 2000 km/s. Out of these, 19 turned out to have been spectroscopically misidentified in…

天体物理学 · 物理学 2009-11-06 M. -P. Veron-Cetty , P. Veron , A. C. Goncalves

We present $J$-band near-infrared (NIR) imaging of the host galaxies of nine narrow-line Seyfert 1 galaxies (NLS1). Based on high-frequency radio observations at 37~GHz, seven of them could host powerful, most likely relativistic jets. Host…

星系天体物理 · 物理学 2018-11-14 Emilia Järvelä , Anne Lähteenmäki , Marco Berton

High resolution MERLIN 5 GHz observations (0.04") of 7 Seyfert galaxies, selected as the ones previously showing evidence of collimated ejection, have been compared with high resolution archive HST data. The radio maps reveal rich…

天体物理学 · 物理学 2009-11-11 E. Xanthopoulos , A. H. Thean , A. Pedlar , A. M. S. Richards

The discovery of gamma-ray emission from 5 radio-loud narrow-line Seyfert 1 galaxies revealed the presence of a possible emerging third class of AGNs with relativistic jets, in addition to blazars and radio galaxies. The existence of…

高能天体物理现象 · 物理学 2019-08-13 F. D'Ammando , M. Orienti , J. Finke , J. Larsson , M. Giroletti

In this work we study the physical and kinematical properties of the emission line region of Seyfert 1.5 galaxy Mrk 817 using three sets of observations, among which are high-resolution spectra obtained with the Isaac Newton Telescope on…

天体物理学 · 物理学 2009-11-11 D. Ilic , L. C. Popovic , E. Bon , E. G. Mediavilla , V. H. Chavushyan

We study the kinematical and brightness evolution of emission line clouds in the narrow line region (NLR) of Seyfert galaxies during the passage of a jet. We derive a critical density above which a cloud remains radiative after compression…

天体物理学 · 物理学 2009-10-30 W. Steffen , J. L. Gomez , A. C. Raga , R. J. R. Williams

We propose two statistical tests to investigate how we see the nuclear region (r < 0.1 pc) of Narrow-Line Seyfert 1 galaxies (NLS1s). 1) The high-ionization nuclear emission-line region (HINER) test: Seyfert 1 galaxies (S1s) have…

天体物理学 · 物理学 2009-10-31 T. Murayama , T. Nagao , Y. Taniguchi

We present the detection of compact radio structures of fourteen radio-loud narrow line Seyfert 1 (NLS1) galaxies from Very Long Baseline Array observations at 5 GHz, which were performed in 2013. While 50\% of the sources of our sample…

星系天体物理 · 物理学 2015-10-14 Minfeng Gu , Yongjun Chen , S. Komossa , Weimin Yuan , Zhi-Qiang Shen , Kiyoaki Wajima , Hongyan Zhou , J. A. Zensus

We have studied the Ly-al, Hbeta, Halpha and Mg II2798 line profiles of the Seyfert 1 galaxy III Zw 2. The shapes of these broad emission lines show evidence of a multicomponent origin and also features which may be identified as the peaks…

天体物理学 · 物理学 2009-11-10 L. C. Popovic , E. G. Mediavilla , E. Bon , N. Stanic , A. Kubicela

Narrow line Seyfert 1 (NLSy1) galaxies constitute a class of active galactic nuclei characterized by the full width at half maximum (FWHM) of the H$\beta$ broad emission line < 2000 km/s and the flux ratio of [O III] to H$\beta$ < 3. Their…

星系天体物理 · 物理学 2017-06-06 Suvendu Rakshit , C. S. Stalin , Hum Chand , Xue-Guang Zhang

According to the unified model of active galactic nuclei, Seyfert 2 galaxies are physically the same as Seyfert 1 objects and they possess a broad-line region (BLR), but it is hidden from the observer due to their orientation. In the past…

星系天体物理 · 物理学 2016-11-17 Georgi P. Petrov

We present new observations of the field surrounding the Seyfert galaxy NGC 7603, where four galaxies with different redshifts--NGC 7603 (z=0.029), NGC 7603B (z=0.057) and two fainter emission line galaxies (z=0.245 and z=0.394)--are…

天体物理学 · 物理学 2009-11-10 M. Lopez-Corredoira , C. M. Gutierrez

Active Galactic Nuclei (AGN) are axisymmetric systems to first order; their observed properties are likely strong functions of inclination with respect to our line of sight, yet the specific inclinations of all but a few AGN are generally…

星系天体物理 · 物理学 2015-06-18 T. C. Fischer , D. M. Crenshaw , S. B. Kraemer , H. R. Schmitt , T. J. Turner