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相关论文: The Close Environment of Seyfert Galaxies and Its …

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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

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

A technique is described that permits the robust decomposition of the bulge and disk components of a sample of Seyfert galaxies, as well as a (control) sample of non-active galaxies matched to the Seyferts in the distributions of redshift,…

天体物理学 · 物理学 2009-10-31 S. N. Virani , M. M. De Robertis , M. L. VanDalfsen

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

A modification of the popular unification model for Seyfert galaxies is proposed, which takes into account recent observational findings on the statistical properties of both type 1 and type 2 Seyferts. In the proposed scenario,…

天体物理学 · 物理学 2007-05-23 Giorgio Matt

We present a study of the local environment (<200 kpc/h) of 31 Hidden Broad Line Region (HBLR) and 43 non-HBLR Seyfert 2 galaxies (Sy2) in the nearby universe (z<0.04). To compare our findings, we constructed two control samples that match…

星系天体物理 · 物理学 2014-11-11 E. Koulouridis

We have searched for companion galaxies in the close environment of 98 star-forming dwarf galaxies (SFDGs) from field and low density environments, using the NASA Extragalactic Database. Most of the companions are dwarf galaxies which due…

天体物理学 · 物理学 2009-11-06 K. G. Noeske , J. Iglesias-Paramo , J. M. Vilchez , P. Papaderos , K. J. Fricke

Parallel analysis of the large-scale morphology and local environment of matched active and control galaxy samples plays an important role in studies of the fueling of active galactic nuclei. We carry out a detailed morphological…

宇宙学与河外天体物理 · 物理学 2010-11-09 L. Slavcheva-Mihova , B. Mihov

Using the NASA Extragalactic Database, we have searched the close environment of 98 star-forming dwarf galaxies (SFDGs) from field- and low density environments for companion galaxies. Most of the found companions are dwarf galaxies,…

天体物理学 · 物理学 2007-05-23 K. G. Noeske , J. Iglesias-Paramo , J. M. Vilchez , P. Papaderos , K. J. Fricke

We use a complete AGN sample (Ho et al. 1997) to study the environment of Seyferts, LINERs and HII galaxies. For each AGN we search for companions in the UZC redshift catalogue and compute local as well as large scale neighbour density and…

天体物理学 · 物理学 2007-05-23 V. Zitelli , B. Kelm , P. Focardi , S. Montanaro

In this paper we present a statistical study of the environments of 49 galaxies in which there is gas- or stellar- counterrotation. The number of possible companions in the field (to apparent magnitude 22), their size and concentration were…

天体物理学 · 物理学 2009-11-06 D. Bettoni , G. Galletta , F. Prada

We study the environment of active galaxies and compare it with that of star forming and normal galaxies. We extracted from the Fourth Data Release (DR4) of the Sloan Digitaly Sky Survey (SDSS) the galaxies in the redshift range 0.05 \le z…

天体物理学 · 物理学 2007-05-23 G. Sorrentino , M. Radovich , A. Rifatto

This paper studies systematically, for the first time, the circumgalactic environment of bright IRAS galaxies as defined by Soifer et al. (1989). While the role of gravitational interaction for luminous and ultraluminous IRAS galaxies has…

天体物理学 · 物理学 2009-11-07 Y. Krongold , Dultzin-Hacyan , P. Marziani

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 results concerning the occurrence of Seyfert galaxies in a new automatically selected sample of nearby Compact Groups of galaxies (UZC-CGs). Seventeen Seyferts are found, constituting ~3% of the UZC-CG galaxy population. CGs…

天体物理学 · 物理学 2009-11-10 B. Kelm , P. Focardi , V. Zitelli

We use the database from Paper III to quantify the global and nuclear properties of emission-line nuclei in the Palomar spectroscopic survey of nearby galaxies. We show that the host galaxies of Seyferts, LINERs, and transition objects…

天体物理学 · 物理学 2009-11-07 Luis C. Ho , Alexei V. Filippenko , Wallace L. W. Sargent

Based on SDSS data, we have considered the spatial environment of galaxies with extended polar rings. We used two approaches: estimating the projected distance to the nearest companion and counting the number of companions as a function of…

星系天体物理 · 物理学 2017-03-22 S. S. Savchenko , V. P. Reshetnikov

A statistical study of the environment around Polar Ring Galaxies is presented. Two kinds of search are performed: 1) a study of the concentration and diameters of all the objects surrounding the Polar Rings, within a search field 5 times…

天体物理学 · 物理学 2007-05-23 Chiara Brocca , Daniela Bettoni , Giuseppe Galletta

We analyse different properties of the small scale environment of Seyfert 2 for two samples selected according to the accretion rate parameter, R, from the DR7-SDSS survey. We compare the results with two control samples of non-active…

宇宙学与河外天体物理 · 物理学 2015-06-17 Georgina V. Coldwell , Sebastian Gurovich , Jorge Diaz Tello , Ilona K. Soechting , Diego G. Lambas

We present a study of the environment of barred galaxies using galaxies drawn from the SDSS. We use several different statistics to quantify the environment: the projected two-point cross-correlation function, the background-subtracted…

星系天体物理 · 物理学 2016-06-29 Bernardo Cervantes Sodi , Cheng Li , Changbom Park , Lixin Wang
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