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相关论文: An Investigation into the Geometry of Seyfert Gala…

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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

We use the difference (delta) between the position angles of the nuclear radio emission and the host galaxy major axis to investigate the distribution of the angle (beta) between the axes of the nuclear accretion disk and the host galaxy…

天体物理学 · 物理学 2009-10-31 Neil M. Nagar , Andrew S. Wilson

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 present a series of statistical tests done to a sample of 29 Seyfert 1 and 59 Seyfert 2 galaxies selected from mostly isotropic properties, their far infrared fluxes and warm infrared colors. Such selection criteria provide a profound…

天体物理学 · 物理学 2009-11-06 H. R. Schmitt , R. R. J. Antonucci , J. S. Ulvestad , A. L. Kinney , C. J. Clarke , J. E. Pringle

We demonstrate that, by combining optical, radio and X-ray observations of a Seyfert, it is possible to provide a direct measurement of the angle $\beta$ between the direction of the radio jet and the normal to the plane of the spiral host…

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

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 preliminary results of the analysis of optical spectra of two complementary samples of Seyfert galaxies. The first sample was extracted from a selection of the 4th Fermi Gamma-ray Large Area Telescope (4FGL) catalog, and consists…

星系天体物理 · 物理学 2023-11-06 Benedetta Dalla Barba , Marco Berton , Luigi Foschini , Giovanni La Mura , Amelia Vietri , Stefano Ciroi

Various models of structure formation can account for various aspects of the galaxy formation process on different scales, as well as for various observational features of structures. Thus, the investigation of galaxies orientation…

星系天体物理 · 物理学 2019-05-01 Paulina Pajowska , Wlodzimierz Godlowski , Zong-Hong Zhu , Joanna Popiela , Elena Panko , Piotr Flin

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

The magnitude-limited catalog of the Southern Sky Redshift Survey (SSRS2), is used to characterize the properties of galaxies hosting Active Galactic Nuclei. Using emission-line ratios, we identify a total of 162 (3%) Seyfert galaxies out…

天体物理学 · 物理学 2009-11-10 Marcio A. G. Maia , Rodolfo S. Machado , Christopher N. A. Willmer

We present the results on an XMM-Newton systematic analysis of a sample of nine Seyfert 1 galaxies. When observed in polarised light, the spectra of the selected sources are similar to those of Seyfert 2 galaxies. This peculiarity strongly…

We analyse the distribution of position angles of 1 million galaxies from the Hyperleda catalogue, a sample that presents the galaxies coordinates in the celestial sphere, information that allows us to look for a possible privileged…

宇宙学与河外天体物理 · 物理学 2017-05-08 R. S. Menezes , C. Pigozzo , S. Carneiro

To understand the origin of radio emission in radio-quiet AGN and differentiate between the contributions from star formation, AGN accretion, and jets, we have observed a nearby sample of Seyfert galaxies along with a comparison sample of…

星系天体物理 · 物理学 2020-10-14 Biny Sebastian , P. Kharb , C. P. O' Dea , J. F. Gallimore , S. A. Baum

The Spitzer high resolution spectra of 72 Seyfert galaxies from the 12$\mu$m Galaxy Sample are presented and discussed. The presence of starburst components in these galaxies can be quantified by powerful mid-IR diagnostics tools (i.e.…

天体物理学 · 物理学 2008-07-31 S. Tommasin , L. Spinoglio , K. Hainline , M. A. Malkan , H. Smith

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 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…

The revision of the fourth Fermi Large Area Telescope (LAT) catalog of gamma-ray point sources (rev4FGL) revealed that the gamma-ray sky is populated by emerging populations of jetted active galactic nuclei (AGN) other than blazars and…

高能天体物理现象 · 物理学 2026-01-27 Luigi Foschini

Seyfert-type AGN that exhibit unusually strong and steep soft X-ray spectra are reviewed, building on observations made during the ROSAT all-sky survey. Two individual cases are described in brief detail, both being identified initially in…

天体物理学 · 物理学 2007-05-23 K. A. Pounds , W. N. Brandt

We investigate the properties of the two-dimensional distribution and kinematics of ionised gas and stars in the central kiloparsecs of a matched sample of nearby active (Seyfert) and inactive galaxies, using the SAURON Integral Field Unit…

天体物理学 · 物理学 2009-09-29 Gaelle Dumas , Carole Mundell , Eric Emsellem , Neil Nagar

We present a three-dimensional study of the local (<100 h^-1} kpc) and the large scale (<1 h^{-1} Mpc) environment of the two main types of Seyfert AGN galaxies. For this purpose we use 48 Sy1 galaxies (with redshifts in the range…

天体物理学 · 物理学 2009-11-13 E. Koulouridis , M. Plionis , V. Chavushyan , D. Dultzin-Hacyan , Y. Krongold , C. Goudis
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