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Related papers: Unveiling the Active Nucleus of Centaurus A

200 papers

High-resolution observations in the near infrared show star clusters around the active galactic nucleus (AGN) of the Seyfert 1 NGC2110, along with a 90 x 35 pc bar of shocked gas material around its nucleus. These are seen for the first…

Astrophysics of Galaxies · Physics 2015-06-18 Mark Durré , Jeremy Mould

Between 2019 and 2024, we used the Gemini-N and JWST observatories to conduct a detailed case study of the active Centaur 450P/LONEOS, whose orbit was significantly altered by a close Saturn encounter in 1992. Gemini-N GMOS optical images…

We present a HST/STIS spectroscopic and optical/radio imaging study of the Seyfert NGC 2110 aiming to measure the dynamics and understand the nature of the nuclear outflow in the galaxy. Previous HST studies have revealed the presence of a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 D. J. Rosario , M. Whittle , C. H. Nelson , A. S. Wilson

Pierre Auger observatory reported the distribution of arrival directions of the highest energy cosmic rays. These events were collected in 10 years of operations with declinations between -90$^\circ$ and +45$^\circ$. The IceCube neutrino…

High Energy Astrophysical Phenomena · Physics 2018-10-17 N. Fraija , E. Aguilar-Ruiz , A. Galván-Gámez , A. Marinelli , J. A. de Diego

We present results from new Chandra and archival HST and VLA imaging observations of the circumnuclear extended emission in the nearby Type 2 Seyfert galaxy NGC 2110. We find resolved soft-band X-ray emission 4'' (~160 pc) north of the…

A 45 deg2 radio continuum imaging campaign of the nearest radio galaxy, Centaurus A, is reported. Using the Australia Telescope Compact Array and the Parkes 64m radio telescope at 1.4 GHz, the spatial resolution of the resultant image is…

High resolution submm observations are important in probing the morphology, column density and dynamics of obscured active galactic nuclei (AGNs). With high resolution (0.06 x 0.05) ALMA 690 GHz observations we have found bright (TB >80 K)…

We present Chandra, Very Large Array (VLA), and Very Long Baseline Array (VLBA) observations of the nucleus of NGC 4696, a giant elliptical in the Centaurus cluster of galaxies. Like M87 in the Virgo cluster, PKS 1246-410 in the Centaurus…

Astrophysics · Physics 2009-09-17 G. B. Taylor , J. S. Sanders , A. C. Fabian , S. W. Allen

The ultraluminous infrared galaxy IRAS 17208$-$0014 is a late-stage merger that hosts a buried active galactic nucleus (AGN). To investigate its nuclear structure, we performed high spatial resolution…

Context. Cygnus A, as the nearest powerful FR II radio galaxy, plays an important role in understanding jets and their impact on the surrounding intracluster medium. Aims. To explain why the nucleus is observed superposed onto the eastern…

Astrophysics of Galaxies · Physics 2015-06-18 K. C. Steenbrugge , K. M. Blundell , S. Pyrzas

The cold molecular gas in the circumnuclear disk (CND) of radio galaxies provides critical information for understanding the mass accretion onto active galactic nuclei. We present the first detection and maps of HCN J=1-0 and HCO+ J=1-0…

Astrophysics of Galaxies · Physics 2022-08-17 Satoko Sawada-Satoh , Seiji Kameno , Sascha Trippe

The S0 galaxy NGC 3245 contains a circumnuclear disk of ionized gas and dust with a radius of 1.1" (110 pc), making it an ideal target for dynamical studies with the Hubble Space Telescope. We have obtained spectra of the nuclear disk with…

Astrophysics · Physics 2009-10-31 A. J. Barth , M. Sarzi , H. -W. Rix , L. C. Ho , A. V. Filippenko , W. L. W. Sargent

In this paper, we report VLBA radio maps at three frequencies and an ASCA X-ray spectrum of the water megamaser galaxy NGC 2639, which is believed to contain an edge-on viewed accretion disk. The radio observations reveal a compact ($<$ 0.2…

We present new HST/STIS observations of Centaurus A. [SIII] 9533A was used to study the kinematics in the nuclear region with a 0.1" spatial resolution. The STIS data and the VLT/ISAAC spectra by Marconi et al. (2001) provide independent…

We present optical images of the nucleus of the nearby radio galaxy M84 (NGC 4374 = 3C272.1) obtained with the Wide Field/Planetary Camera 2 (WFPC2) aboard the Hubble Space Telescope (HST). Our three images cover the H$\alpha$ + [N II]…

Astrophysics · Physics 2016-08-30 Gary A. Bower , Timothy M. Heckman , Andrew S. Wilson , Douglas O. Richstone

We combine Chandra and XMM-Newton X-ray data from our previous papers with new X-ray observations and with Spitzer mid-infrared data in order to study the nature of the nuclei of radio galaxies and radio-loud quasars with z<1.0 from the…

Astrophysics of Galaxies · Physics 2015-05-13 M. J. Hardcastle , D. A. Evans , J. H. Croston

(Abridged) With infrared interferometry it is possible to resolve the nuclear dust distributions that are commonly associated with the dusty torus in active galactic nuclei (AGN). The Circinus galaxy hosts the closest Seyfert 2 nucleus and…

Astrophysics of Galaxies · Physics 2013-12-18 K. R. W. Tristram , L. Burtscher , W. Jaffe , K. Meisenheimer , S. F. Hönig , M. Kishimoto , M. Schartmann , G. Weigelt

The galaxy NGC 4418 contains one of the most compact obscured nuclei within a luminous infrared galaxy (LIRG) in the nearby Universe. This nucleus contains a rich molecular gas environment and an unusually high ratio of infrared to radio…

Astrophysics of Galaxies · Physics 2014-06-04 E. Varenius , J. E. Conway , I. Martí-Vidal , S. Aalto , R. Beswick , F. Costagliola , H. -R. Klöckner

As the closest radio galaxy, Centaurus A is a powerful laboratory for the X-ray study of radio-emitting structures and their interactions with the hot interstellar medium (ISM). This paper details our interpretation of the remarkable X-ray…

In spite of increasing evidences of the presence of a massive Black Hole at the Galactic Center, its radio counterpart, Sgr A*, shows little activity at high energies, and recent models involving energy advection (ADAF) have been proposed…

Astrophysics · Physics 2007-05-23 A. Goldwurm , P. Goldoni , P. Laurent , F. Lebrun , J. Paul