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相关论文: The complex structure of low luminosity AGN : NGC …

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The aim of this study is to constrain the dynamics, structure and feeding of the compact nucleous of NGC4418, and to reveal the nature of the main hidden power source: starburst or AGN. We obtained high spatial resolution observations of…

星系天体物理 · 物理学 2015-06-16 F. Costagliola , S. Aalto , K. Sakamoto , S. Martín , R. Beswick , S. Muller , H. -R. Klöckner

We study the broad-band spectral energy distribution (SED) of the prototypical low-mass active galactic nucleus (AGN) in NGC 4395. We jointly model the optical through mid-infrared SED with a combination of galaxy and AGN light, and find…

星系天体物理 · 物理学 2023-07-31 Hector Afonso G. Cruz , Andy D. Goulding , Jenny E. Greene

NGC 4527 is a nearby edge-on spiral galaxy with both starburst and AGN features, hosting a LINER nucleus. We present a radio study of the large-scale structure and nuclear region of this galaxy, based on new uGMRT observations at 700 and…

星系天体物理 · 物理学 2025-09-03 C. A. Galante , G. E. Romero , J. Saponara , P. Benaglia

We present near-infrared VLT ISAAC imaging and spectroscopy of the peculiar Virgo galaxy NGC 4438, whose nucleus has been classified as a LINER. The data are supplemented by mid-infrared imaging, and compared to previous WFPC2 HST broadband…

星系天体物理 · 物理学 2015-05-14 Sebastian Perez , Simon Casassus , Juan R. Cortes , J. D. P. Kenney

We study the extended nuclear emission of the starburst galaxy NGC 1365. A weak obscured AGN and a strong starburst both contribute to the observed X-ray, optical, infrared, and radio emission in the inner 2kpc. The X-ray emission is…

高能天体物理现象 · 物理学 2009-03-10 I. V. Strateva , S. Komossa

Observations of the Seyfert 2 and starburst galaxy NGC 5135 with the Chandra X-ray Observatory demonstrate that both of these phenomena contribute significantly to its X-ray emission. We spatially isolate the active galactic nucleus (AGN)…

天体物理学 · 物理学 2016-08-30 N. A. Levenson , K. A. Weaver , T. M. Heckman , H. Awaki , Y. Terashima

Galaxies which strongly deviate from the radio-far IR correlation are of great importance for studies of galaxy evolution as they may be tracing early, short-lived stages of starbursts and active galactic nuclei (AGNs). The most extreme…

星系天体物理 · 物理学 2016-10-26 F. Costagliola , R. Herrero-Illana , A. Lohfink , M. Pérez-Torres , S. Aalto , S. Muller , A. Alberdi

The Large High Altitude Air Shower Observatory has detected very high-energy (VHE) gamma rays from NGC 4278, which is known to host a low-luminosity active galactic nucleus (AGN). Having only very weak radio jets, the origin of its VHE…

高能天体物理现象 · 物理学 2025-11-11 Asahi Shoji , Yutaka Fujita , Norita Kawanaka , Susumu Inoue , Kosuke Nishiwaki

The low-luminosity active galactic nuclei in NGC 3147, NGC 4203, and NGC 4579 have been imaged at four frequencies with the Very Long Baseline Array. The galaxies are unresolved at all frequencies, with size upper limits of $10^3-10^4$…

天体物理学 · 物理学 2009-11-07 James S. Ulvestad , Luis C. Ho

We have compiled a new multiwavelength spectral energy distribution (SED) for the closest obscured low-ionization emission-line region active galactic nucleus (AGN), NGC 4736, also known as M94. The SED comprises mainly high-resolution…

高能天体物理现象 · 物理学 2017-04-20 Pieter van Oers , Sera Markoff , Phil Uttley , Ian McHardy , Tessel van der Laan , Jennifer Donovan Meyer , Riley Connors

The X-ray properties of 15 nearby (v<3,000 km/s) galaxies that possess AGN and/or starbursts are discussed. Two-thirds have nuclear extended emission on scales from ~0.5 to ~1.5 kpc that is either clearly associated with a nuclear outflow…

天体物理学 · 物理学 2007-05-23 Kimberly A. Weaver

A multi-cloud model is presented which explains the soft X-ray excess in NGC 4051 and, consistently, the optical line spectrum and the SED of the continuum. The clouds are heated and ionized by the photoionizing flux from the active center…

天体物理学 · 物理学 2009-10-31 M. Contini , S. M. Viegas

We present a deep (~5.8 days) 0.3-2 keV high-resolution spectrum of NGC1365, collected with the reflection grating spectrometer (RGS) on board XMM-Newton. The spectrum is dominated by strong recombination lines of He- and H-like transitions…

宇宙学与河外天体物理 · 物理学 2015-05-13 M. Guainazzi , G. Risaliti , A. Nucita , Junfeng Wang , S. Bianchi , R. Soria , A. Zezas

The nearby low-luminosity active galactic nucleus (LLAGN) NGC 4258 has a weak radio continuum component at the galactic center. We investigate its radio spectral properties on the basis of our new observations using the Nobeyama Millimeter…

星系天体物理 · 物理学 2015-06-12 Akihiro Doi , Kotaro Kohno , Kouichiro Nakanishi , Seiji Kameno , Makoto Inoue , Kazuhiro Hada , Kazuo Sorai

We investigate faint radio emission from low- to high-luminosity Active Galactic Nuclei (AGN) selected from the Sloan Digital Sky Survey (SDSS). Their radio properties are inferred by co-adding large ensembles of radio image cut-outs from…

天体物理学 · 物理学 2008-11-26 W. H. de Vries , J. A. Hodge , R. H. Becker , R. L. White , D. J. Helfand

We analyse two-dimensional near-IR K-band spectra from the inner 660x315 pc^2 of the Seyfert galaxy NGC7582 obtained with the Gemini GNIRS IFU. The nucleus harbors an unresolved source well reproduced by a blackbody of temperature T 1050 K,…

天体物理学 · 物理学 2009-11-13 Rogemar A. Riffel , Thaisa Storchi-Bergmann , Oli L. Dors , Claudia Winge

NGC 1275 is one of the most conspicuous active galactic nuclei (AGN) in the local Universe. The radio jet currently emits a flux density of $\sim 10$ Jy at $\sim 1$ mm wavelengths, down from the historic high of $\sim 65$ Jy in 1980. Yet,…

星系天体物理 · 物理学 2018-12-26 Brian Punsly , Paola Marziani , Vardha N. Bennert , Hiroshi Nagai , Mark A. Gurwell

The multiwavelength emission spectrum and associated velocity field of the Seyfert prototype NGC 4151 is modeled. HST data has impressively revealed the existence of a large range of velocities (100 - 1500 \kms) dominating the emitting…

天体物理学 · 物理学 2009-11-07 M. Contini , S. M. Viegas , M. A. Prieto

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

This is the first paper of a series exploring the multi-frequency properties of a sample of eleven nearby low excitation radio galaxies (LERGs) in the southern sky. We are conducting an extensive study of different galaxy components (stars,…

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