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相关论文: Starburst-AGN mixing: I. NGC 7130

200 篇论文

(Abridged) We examine the power source of 41 local Ultraluminous Infrared Galaxies using archival infrared and optical photometry. We fit the observed Spectral Energy Distributions (SEDs) with starburst and AGN components; each component…

天体物理学 · 物理学 2008-11-26 D. Farrah , J. Afonso , A. Efstathiou , M. Rowan-Robinson , M. Fox , D. Clements

We investigate the fraction of starbursts, starburst-AGN composites, Seyferts, and LINERs as a function of infrared luminosity (L_IR) and merger progress for ~500 infrared-selected galaxies. Using the new optical classifications afforded by…

宇宙学与河外天体物理 · 物理学 2014-11-20 T. -T. Yuan , L. J. Kewley , D. B. Sanders

Observations of the Seyfert 2 and starburst galaxy NGC 7130 with the Chandra X-ray Observatory illustrate that both of these phenomena contribute significantly to the galaxy's detectable X-ray emission. The active galactic nucleus (AGN) is…

天体物理学 · 物理学 2014-10-13 N. A. Levenson , K. A. Weaver , T. M. Heckman , H. Awaki , Y. Terashima

We present a study of the central 2.3 kpc of NGC 5135, a nearby Luminous Infrared Galaxy (LIRG) with an AGN and circumnuclear starburst. Our main results are based on intermediate spectral resolution (~ 3000-4000) near infrared data taken…

宇宙学与河外天体物理 · 物理学 2014-11-18 A. G. Bedregal , L. Colina , A. Alonso-Herrero , S. Arribas

We present sub-mm photometry for 11 Hyperluminous Infrared Galaxies (HLIRGs) and use radiative transfer models for starbursts and AGN to investigate the IR emission. In all sources both a starburst and AGN are required to explain the IR…

天体物理学 · 物理学 2009-11-07 D. Farrah , S. Serjeant , A. Efstathiou , M. Rowan-Robinson , A. Verma

Galaxy mergers are key events in galaxy evolution, often causing massive starbursts and fueling active galactic nuclei (AGN). In these highly dynamic systems, it is not yet precisely known how much starbursts and AGN respectively contribute…

We present Infrared Space Observatory mid- and far-infrared spectroscopy of the merging galaxy NGC 6240, an object presenting many aspects of importance for the role of star formation and AGN activity in [ultra]luminous infrared galaxies.…

天体物理学 · 物理学 2009-11-10 D. Lutz , E. Sturm , R. Genzel , H. W. W. Spoon , A. F. M. Moorwood , H. Netzer , A. Sternberg

AGN are a key ingredient for understanding galactic evolution. AGN-driven outflows are one of the manifestations of feedback. The AO mode for MUSE at the VLT permits to study the innermost tens of parsecs of nearby AGN in the optical. We…

星系天体物理 · 物理学 2021-04-08 S. Comerón , J. H. Knapen , C. Ramos Almeida , A. E. Watkins

We use 4 galaxies from the Calar Alto Legacy Integral Field Area (CALIFA) survey with clear signs of accretion onto supermassive black holes to investigate the relative contribution of star-formation and active galactic nucleus (AGN)…

星系天体物理 · 物理学 2015-06-22 Rebecca L. Davies , Lisa J. Kewley , I-Ting Ho , Michael A. Dopita

Mrk938 is a luminous infrared galaxy in the local Universe believed to be the remnant of a galaxy merger. It shows a Seyfert 2 nucleus and intense star formation according to optical spectroscopic observations. We have studied this galaxy…

Nuclear starbursts and AGN activity are the main heating processes in luminous infrared galaxies (LIRGs) and their relationship is fundamental to understand galaxy evolution. In this paper, we study the star-formation and AGN activity of a…

We apply a simple model, tested on local ULIRGs, to disentangle the active galactic nucleus (AGN) and starburst contributions in submillimiter and 24um-selected ULIRGs observed with the Spitzer-IRS spectrometer. We quantitatively estimate…

宇宙学与河外天体物理 · 物理学 2015-05-13 Y. Watabe , G. Risaliti , M. Salvati , E. Nardini , E. Sani , A. Marconi

Metallicity measurements in galaxies can give valuable clues about galaxy evolution. One of the mechanisms postulated for metallicity redistribution in galaxies is gas flows induced by AGN, but the details of this process remain elusive. We…

星系天体物理 · 物理学 2024-09-18 Amirnezam Amiri , Johan H. Knapen , Sébastien Comerón , Alessandro Marconi , Bret. D. Lehmer

We analyze the link between active galactic nuclei (AGN) and mid-infrared flux using dust radiative transfer calculations of starbursts realized in hydrodynamical simulations. Focusing on the effects of galaxy dust, we evaluate diagnostics…

宇宙学与河外天体物理 · 物理学 2013-07-12 Gregory F. Snyder , Christopher C. Hayward , Anna Sajina , Patrik Jonsson , Thomas J. Cox , Lars Hernquist , Philip F. Hopkins , Lin Yan

We analyze by detailed modelling the spectra observed from the sample galaxies at z$\sim$0.8 presented by Ly et al (2015), constraining the models by the [OIII]5007+4959/[OIII]4363 line ratios. Composite models accounting for shock and…

星系天体物理 · 物理学 2016-07-27 M. Contini

We present the first AGN census in a sample of 61 galaxies selected at 70microns, a wavelength which should strongly favour the detection of star-forming systems. For the purpose of this study we take advantage of deep Chandra X-ray and…

宇宙学与河外天体物理 · 物理学 2015-05-14 M. Symeonidis , D. Rosario , A. Georgakakis , J. Harker , E. S. Laird , M. J. Page

We present the discovery of a small kinematically decoupled core of 0.2$^{\prime\prime}$ (60 pc) in radius as well as an outflow jet in the archetypical AGN-starburst "composite" galaxy NGC 7130 from integral field data obtained with the…

星系天体物理 · 物理学 2019-01-09 J. H. Knapen , S. Comerón , M. K. Seidel

We present a 5-8 micron analysis of the Spitzer-IRS spectra of 71 ultraluminous infrared galaxies (ULIRGs) with redshift z < 0.15, devoted to the study of the role of active galactic nuclei (AGN) and starbursts (SB) as the power source of…

宇宙学与河外天体物理 · 物理学 2015-05-13 E. Nardini , G. Risaliti , M. Salvati , E. Sani , Y. Watabe , A. Marconi , R. Maiolino

We present observations of radio recombination lines from the starburst galaxy Arp 220 at 1.4, 8.1, 84, 96 and 207 GHz (sensitive upper limit for the 1.4 GHz line and firm detections at the other frequencies), and the radio continuum…

天体物理学 · 物理学 2009-10-31 K. R. Anantharamaiah , F. Viallefond , Niruj R. Mohan , W. M. Goss , J. H. Zhao
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