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相关论文: Optical Spectroscopy of nearby type1-LINERs

200 篇论文

We analyze the absorption and emission-line profiles produced by a set of simple, cool gas wind models motivated by galactic-scale outflow observations. We implement monte carlo radiative transfer techniques that track the propagation of…

星系天体物理 · 物理学 2015-05-27 J. Xavier Prochaska , Daniel Kasen , Kate Rubin

The cross-correlation of the Sloan Digital Sky Survey Data Release 7 with the Faint Images of the Radio Sky at Twenty-Centimeters survey allows for a multiwavelength statistical study of radio-optical galaxy properties on a very large…

宇宙学与河外天体物理 · 物理学 2013-03-04 Mariangela Vitale , Jens Zuther , Macarena García-Marín , Andreas Eckart , Marcus Bremer , Mónica Valencia-S , Anton Zensus

We perform a systematic study of outflow in the narrow-line region (NLR) of active galactic nuclei (AGNs) at $z\sim0.4-0.8$ basing upon a large sample of $\sim900$ quasars at $z\sim 0.4-0.8$. The sample is extracted from the Sloan Digital…

星系天体物理 · 物理学 2018-01-10 J. Wang , D. W. Xu , J. Y. Wei

We present near infrared ISAAC VLT observations of nine (0.01<z<0.06) Active Galactic Nuclei selected from the Hamburg/ESO Survey and the Veron-Cetty & Veron catalog. Hydrogen recombination lines Pa$\alpha$ and Br$\gamma$ are observed in…

天体物理学 · 物理学 2009-11-11 S. Fischer , C. Iserlohe , J. Zuther , T. Bertram , C. Straubmeier , R. Schoedel , A. Eckart

In this work, we investigated the nitrogen and oxygen abundances in a sample of galaxies with Low Ionization Nuclear Emission Regions (LINERs) in their nucleus. Optical spectroscopic data (3 600 - 10 000 {\AA}) of 40 LINERs from the Mapping…

This paper reports the results of a near infrared spectroscopic survey of LINER galaxies undertaken with a new infrared spectrograph at the 5 m Hale telescope. The galaxy sample includes 11 LINERs with spectra covering the [FeII] (1.2567…

天体物理学 · 物理学 2009-10-30 J. E. Larkin , L. Armus , R. A. Knop , B. T. Soifer , K. Matthews

We study a complete and distance-limited sample of 25 LINERs, 21 of which have been imaged with the Hubble Space Telescope. In nine objects we detect an unresolved nucleus. In order to study their physical properties, we compare the radio…

天体物理学 · 物理学 2009-11-10 Marco Chiaberge , Alessandro Capetti , F. Duccio Macchetto

We analyze a set of optical-to-near-infrared long-slit nuclear spectra of 16 infrared-luminous spiral galaxies. All of the studied sources present H$_2$ emission, which reflects the star-forming nature of our sample, and they clearly…

We present the results of an homogeneous X-ray analysis for 82 nearby LINERs selected from the catalogue of Carrillo et al. (1999). All sources have available Chandra (68 sources) and/or XMM-Newton (55 sources) observations. This is the…

宇宙学与河外天体物理 · 物理学 2015-05-13 O. Gonzalez-Martin , J. Masegosa , I. Marquez , M. Guainazzi , E. Jimenez-Bailon

Objective-prism surveys for UV-excess and emission-line objects, especially the First and Second Byurakan Surveys, have been central to the study of active galactic nuclei (AGNs). We review previous line-selected surveys for AGNs and…

天体物理学 · 物理学 2007-05-23 Caryl Gronwall , Vicki Sarajedini , John Salzer

We present a study of available Hubble Space Telescope (HST) spectroscopic and imaging observations of the low ionization nuclear emission line region (LINER) galaxy NGC 1052. The WFPC2 imagery clearly differentiates extended nebular Halpha…

天体物理学 · 物理学 2009-10-31 J. R. Gabel , F. C. Bruhweiler , D. M. Crenshaw , S. B. Kraemer , C. L. Miskey

The origin of the low-ionization nuclear emission-line region (LINER) prevalent in local galaxies and its relationship with supermassive black holes are debated for decades. We preform a comprehensive evaluation of traditional…

星系天体物理 · 物理学 2023-10-12 Zongnan Li , Zhiyuan Li , Ruben Garcia-Benito , Yifei Jin

The results of Chandra snapshot observations of 11 LINERs (Low-Ionization Nuclear Emission-line Regions), three low-luminosity Seyfert galaxies, and one HII-LINER transition object are presented. Our sample consists of all the objects with…

天体物理学 · 物理学 2007-05-23 Yuichi Terashima , Andrew S. Wilson

In this work we investigate the properties of the broad emission line components in the Balmer series of a sample of Type 1 Active Galactic Nuclei (AGN). Using the Boltzmann Plot method as a diagnostic tool for physical conditions in the…

宇宙学与河外天体物理 · 物理学 2014-11-20 G. La Mura , F. Di Mille , L. Č. Popović , S. Ciroi , P. Rafanelli , D. Ilić

We analyze the properties of the innermost narrow line region in a sample of low-luminosity AGN. We select 33 LINERs (bona fide AGN) and Seyfert galaxies from the optical spectroscopic Palomar survey observed by HST/STIS. We find that in…

星系天体物理 · 物理学 2016-01-27 B. Balmaverde , A. Capetti , D. Moisio , R. D. Baldi , A. Marconi

Outflows play a major role in the evolution of galaxies. However, we do not have yet a complete picture of their properties (extension, geometry, orientation and clumpiness). For low-luminosity Active Galactic Nuclei (AGNs), in particular,…

星系天体物理 · 物理学 2022-04-27 Laura Hermosa Muñoz , Isabel Márquez , Sara Cazzoli , Josefa Masegosa , Beatriz Agís-González

We present an investigation of the structure of the emission line region in a sample of 12 single-peaked Active Galactic Nuclei (AGNs). Using the high resolution H-beta and H-alpha line profiles observed with the Isaac Newton Telescope (La…

天体物理学 · 物理学 2009-11-10 L. C. Popovic , E. Mediavilla , E. Bon , D. Ilic

We present detailed image analysis of rest-frame optical images of 235 low-redshift ($z \leq$ 0.35) type 1 active galactic nuclei (AGNs) observed with the Hubble Space Telescope. The high-resolution images enable us to perform rigorous…

星系天体物理 · 物理学 2017-10-09 Minjin Kim , Luis C. Ho , Chien Y. Peng , Aaron J. Barth , Myungshin Im

Historically, the study of the central regions of Type 1 AGN has been limited by the combination of the host galaxy spectrum with strong emission from the accretion disk and NLR/BLR, which prevented us from accurately probing the galactic…

We present new optical and infrared (IR) observations of Cir X-1 taken near apastron. Both sets of spectra show asymmetric emission lines. Archival optical observations show that an asymmetric H-alpha emission line has been in evidence for…

天体物理学 · 物理学 2009-10-31 Helen Johnston , Rob Fender , Kinwah Wu