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相关论文: Centaurus A - NGC 5128

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We report new HST WFPC2 and NICMOS observations of the center of the nearest radio galaxy Centaurus A (NGC 5128) and discuss their implications for our understanding of the active nucleus and jet. We detect the active nucleus in the near-IR…

The Centaurus A radio galaxy, due to its proximity, presents itself as one of the few systems that allow the study of relativistic jet outflows at sub-parsec distances from the central supermassive black holes, with high signal to noise. We…

高能天体物理现象 · 物理学 2024-12-03 Steve Prabu , Steven J Tingay , Arash Bahramian , James C. A. Miller-Jones , Callan M. Wood , Shane P. O'Sullivan

At less than 4 Mpc distance the radio galaxy NGC 5128 (Centaurus A) is the prime example to study the supermassive black hole and its influence on the environment in great detail. To model and understand the feeding and feedback mechanisms…

宇宙学与河外天体物理 · 物理学 2015-05-18 Nadine Neumayer

Giant radio galaxies are thought to be massive ellipticals powered by accretion of interstellar matter onto a supermassive black hole. Interactions with gas rich galaxies may provide the interstellar matter to feed the active galactic…

天体物理学 · 物理学 2007-05-23 I. F. Mirabel , O. Laurent

The infrared spectrograph GNIRS on Gemini South unlocks new possibilities to study the central black holes in dusty galaxies that have been inaccessible to previous black hole studies. We exploit good near-infrared seeing to measure the…

天体物理学 · 物理学 2009-11-10 Julia D. Silge , Karl Gebhardt , Marcel Bergmann , Douglas Richstone

We present new ATCA 21-cm line observations of the neutral hydrogen in the nearby radio galaxy Centaurus A. We image in detail (with a resolution down to 7", ~100pc) the distribution of HI along the dust lane. Our data have better velocity…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. Struve , T. A. Oosterloo , R. Morganti , L. Saripalli

We describe results from our initial study of the diffuse X-ray emission structures in NGC 5128 (Cen A) using the Chandra X-ray Observatory observations. The high-angular resolution Chandra images reveal multi-scale X-ray struct ures with…

天体物理学 · 物理学 2009-11-07 M. Karovska , G. Fabbiano , F. Nicastro , M. Elvis , R. P. Kraft , S. S. Murray

We present deep radio images of the inner 50 kpc of Centaurus A, taken with the Karl G. Jansky Very Large Array (VLA) at 90cm. We focus on the Transition Regions between the inner galaxy - including the active nucleus, inner radio lobes,…

星系天体物理 · 物理学 2015-06-23 Susan G. Neff , Jean A. Eilek , Frazer N. Owen

For the first time, systematic studies of dwarf galaxies are being conducted throughout the Local Volume, including the dwarf satellites of the nearby giant elliptical galaxy Centaurus A (NGC 5128). Given Centaurus As mass (roughly ten…

星系天体物理 · 物理学 2024-12-04 Sachi Weerasooriya , Mia Sauda Bovill , Matthew A. Taylor , Andrew J. Benson , Cameron Leahy

NGC 5128 (Centaurus A) is, at the distance of just 3.8 Mpc, the nearest easily observable giant elliptical galaxy. Therefore it is the best target to investigate the early star formation history of an elliptical galaxy. Our aims are to…

宇宙学与河外天体物理 · 物理学 2015-05-20 M. Rejkuba , W. E. Harris , L. Greggio , G. L. H. Harris

We present a study of the nearby post-merger giant elliptical galaxy, NGC 5128 (Centaurus A), in which we use the properties of its globular cluster (GC) and planetary nebula (PN) systems to constrain its evolution. Using photometric and…

天体物理学 · 物理学 2009-11-10 Eric W. Peng , Holland C. Ford , Kenneth C. Freeman

We present results from a sensitive high-resolution X-ray observation of the nearby active galaxy Centaurus A (NGC 5128) with the ROSAT HRI. The 65~ksec X-ray image clearly distinguishes different components of the X-ray emission from Cen…

天体物理学 · 物理学 2009-10-28 S. Doebereiner , N. Junkes , S. J. Wagner , H. Zinnecker , R. Fosbury , G. Fabbiano , E. J. Schreier

We have analysed a new high-resolution e-MERLIN 1.5 GHz radio continuum map together with $HST$ and SDSS imaging of NGC 5322, an elliptical galaxy hosting radio jets, aiming to understand the galaxy's central structure and its connection to…

We present ALMA CO(1-0) observations toward the dust lane of the nearest elliptical and radio galaxy, NGC 5128 (Centaurus A), with high angular resolution ($\sim$ 1 arcsec, or 18 pc), including information from large to small spatial scales…

We report on atomic gas (HI) and molecular gas (as traced by CO(2-1)) redshifted absorption features toward the nuclear regions of the closest powerful radio galaxy, Centaurus A (NGC 5128). Our HI observations using the Very Long Baseline…

宇宙学与河外天体物理 · 物理学 2015-05-19 D. Espada , A. B. Peck , S. Matsushita , K. Sakamoto , C. Henkel , D. Iono , F. P. Israel , S. Muller , G. Petitpas , Y. Pihlstroem , G. B. Taylor , D. V. Trung

The study of planetary nebulae (PNe) in the nearby post-merger elliptical galaxy NGC 5128 (Cen A) now has a history of nearly twenty years. As the nearest giant elliptical, it is a prime target for extragalactic PN studies. These studies…

天体物理学 · 物理学 2007-05-23 Eric W. Peng , Holland C. Ford , Kenneth C. Freeman

In a study of the radio emission mechanism of the FR-I AGN NGC 5128 (Centaurus A)}, we have determined the centimeter and millimeter continuum spectrum of the whole Centaurus A radio source and measured the continuum emission from the…

天体物理学 · 物理学 2009-11-13 F. P. Israel , D. Raban , R. S. Booth , F. T. Rantakyro

NGC 5128 (Cen A) is the nearest giant elliptical galaxy and one of the brightest extragalactic radio sources in the sky, boasting a prominent dust lane and jets emanating from its nuclear supermassive black hole. In this paper, we construct…

The physical state of the gas in the central 500 pc of NGC~5128 (the radio galaxy Centaurus A - Cen A), was investigated using the far-infrared fine-structure lines of carbon, oxygen, and nitrogen, as well as the CO(4-3) molecular line. The…

星系天体物理 · 物理学 2017-03-01 F. P. Israel , R. Guesten , R. Meijerink , M. A. Requena-Torres , J. Stutzki

We report the discovery of an extended globular cluster in a halo field in Centaurus A (NGC 5128), situated $\sim 38\kpc$ from the centre of that galaxy, imaged with the Advanced Camera for Surveys on board the Hubble Space Telescope. At…

星系天体物理 · 物理学 2015-05-18 M. Mouhcine , W. E. Harris , R. Ibata , M. Rejkuba