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相关论文: Testing the Unified Model with an Infrared Selecte…

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We present a series of statistical tests using homogeneous data and measurements for a sample of Seyfert galaxies. These galaxies were selected from mostly isotropic properties, their far infrared fluxes and warm infrared colors, which…

天体物理学 · 物理学 2007-05-23 H. R. Schmitt , J. S. Ulvestad , R. R. J. Antonucci , C. J. Clarke , J. E. Pringle , A. L. Kinney

We use the radio axis as an indicator of the orientation of the obscuring torus in Seyfert galaxies, and analyze the difference between the position angles of extended radio structures and host galaxy major axis of Seyfert 1 and Seyfert 2…

天体物理学 · 物理学 2009-10-28 H. R. Schmitt , A. L. Kinney , T. Storchi-Bergmann , R. Antonucci

We studied the physical parameters of a sample comprising of all Spitzer/IRS public spectra of Seyfert galaxies in the mid-infrared (5.2-38$\mu$m range) under the active galactic nuclei (AGN) unified model. We compare the observed spectra…

We present new mid-infrared (MIR) imaging data for three Type-1 Seyfert galaxies obtained with T-ReCS on the Gemini-South Telescope at subarcsecond resolution. Our aim is to enlarge the sample studied in a previous work to compare the…

This paper presents a statistical analysis of the circumgalactic environment of nearby Seyfert galaxies based on a computer-aided search of companion galaxies on the Digitized Sky Survey (DSS). An intrinsic difference between the…

天体物理学 · 物理学 2009-10-31 D. Dultzin-Hacyan , Y. Krongold , I. Fuentes-Guridi , P. Marziani

We present the results of broad-band B and I imaging observations for a sample of 88 Seyfert galaxies (29 Seyfert 1's and 59 Seyfert 2's), selected from a mostly isotropic property, the flux at 60$\mu$m. We also present the B and I imaging…

天体物理学 · 物理学 2009-10-31 H. R. Schmitt , A. L. Kinney

We have carried out an analysis of the radio and optical properties of a statistical sample of 45 Seyfert galaxies from the Palomar spectroscopic survey of nearby galaxies. We find that the space density of bright galaxies (-22 mag <=…

天体物理学 · 物理学 2009-11-06 James S. Ulvestad , Luis C. Ho

The infrared is a key wavelength regime for probing the dusty, obscured nuclear regions of active galaxies. We present results from an infrared study of 87 nearby Seyfert galaxies using the Spitzer Space Telescope and ground-based…

(Abbreviated) We assemble a sample composed of 243 nearby Seyfert galaxies with redshifts $z\le 0.05$ to test the unification scheme. The sample contains 94 BLS1s, 44 NLS1s, 36 X-ray absorbed HBLR S2s, 42 X-ray absorbed non-HBLR S2s and 27…

天体物理学 · 物理学 2011-02-11 Jian-Min Wang , En-Peng Zhang

We used the CLUMPY torus models and a Bayesian approach to fit the infrared spectral energy distributions (SEDs) and ground-based high-angular resolution mid-infrared spectroscopy of 13 nearby Seyfert galaxies. This allowed us to put tight…

We present a new method for the statistical investigation into the distributions of the angle beta between the radio axis and the normal to the galactic disk for a sample of Seyfert galaxies. We discuss how further observations of the…

天体物理学 · 物理学 2009-10-30 C. J. Clarke , A. L. Kinney , J. E. Pringle

We have identified 12 Seyfert 1 galaxies that exhibit optical polarization spectra similar to those of Seyfert 2 galaxies in which polarized broad-lines are detected. We present new spectropolarimetric observations of 3 of them: Was 45, Mrk…

天体物理学 · 物理学 2008-11-26 J. E. Smith , A. Robinson , D. M. Alexander , S. Young , D. J. Axon , Elizabeth A. Corbett

A radio study of a carefully selected sample of 20 Seyfert galaxies that are matched in orientation-independent parameters, which are measures of intrinsic active galactic nuclei (AGN) power and host galaxy properties is presented to test…

宇宙学与河外天体物理 · 物理学 2015-05-27 Dharam V. Lal , Prajval Shastri , Denise Gabuzda

We present near-to-mid-infrared spectral energy distributions (SEDs) for 21 Seyfert galaxies, using subarcsecond resolution imaging data. Our aim is to compare the properties Seyfert 1 (Sy1) and Seyfert 2 (Sy2) tori using clumpy torus…

We performed imaging on 49 type 2 Seyfert galaxies in 6 near- and mid-infrared bands (1-10$\mu$m). We are separating the contribution of the torus from the host galaxy by radial profile fitting techniques and we will compare the observed…

天体物理学 · 物理学 2007-05-23 L. Videla , P. Lira , A. Alonso-Herrero , D. M. Alexander , M. Ward

New far-infrared photometry with ISOPHOT, onboard the Infrared Space Observatory, is presented for 58 galaxies with homogeneous published data for another 32 galaxies all belonging to the 12 micron galaxy sample. In total 29 Seyfert 1's, 35…

天体物理学 · 物理学 2009-11-07 Luigi Spinoglio , Paola Andreani , Matthew A. Malkan

We have observed a sample of Seyfert (Sy) galaxies with the global Very Long Baseline Interferometry (VLBI) to test the predictions of the unification scheme for the Sy galaxies which hypothesises that Sys of Type 1 and of Type 2 constitute…

天体物理学 · 物理学 2007-05-23 Dharam Vir Lal

We present the results of VLA A-array 8.46 GHz continuum imaging of 55 Seyfert galaxies (19 Seyfert 1's and 36 Seyfert 2's). These galaxies are part of a larger sample of 88 Seyfert galaxies, selected from mostly isotropic properties, the…

天体物理学 · 物理学 2009-10-31 H. R. Schmitt , J. S. Ulvestad , R. R. J. Antonucci , A. L. Kinney

We present the results of a Hubble Space Telescope (HST) survey of extended [OIII] emission in a sample of 60 nearby Seyfert galaxies (22 Seyfert 1's and 38 Seyfert 2's), selected by mostly isotropic properties. The comparison between the…

天体物理学 · 物理学 2009-11-10 H. R. Schmitt , J. L. Donley , R. R. J. Antonucci , J. B. Hutchings , A. L. Kinney , J. E. Pringle

We present the study of the relative angle between the accretion disk (or radio jet) and the galaxy disk for a sample of Seyfert galaxies selected from a mostly isotropic property, the 60$\mu$m flux. For each galaxy we have a pair of points…

天体物理学 · 物理学 2010-12-09 A. L. Kinney , H. R. Schmitt , C. J. Clarke , J. E. Pringle , J. S. Ulvestad , R. R. J. Antonucci
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