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相关论文: Polarization and kinematics in Cygnus A

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We use Gemini Near-Infrared Integral Field Spectrograph (NIFS) observations of the inner 3.5$\times$3.5 kpc$^2$ of the radio galaxy Cygnus A to map the gas excitation and kinematics at a spatial resolution of 200 pc. The emission of the…

星系天体物理 · 物理学 2022-08-31 Rogemar A. Riffel

We report the detection of linearly polarized emission at 53 and 89 $\mu$m, from the radio-loud active galactic nucleus (AGN) Cygnus A using HAWC+ onboard SOFIA. We measure a highly polarized core of $11\pm3$% and $9\pm2$% with a position…

星系天体物理 · 物理学 2018-07-25 Enrique Lopez-Rodriguez , Robert Antonucci , Ranga-ram Chary , Makoto Kishimoto

We present near-IR imaging polarimetry observations of the nucleus of Cygnus A, taken with the NICMOS camera of the HST at a wavelength of 2.0 microns.These maps reveal a highly collimated region of polarized emission straddling the nucleus…

天体物理学 · 物理学 2009-10-31 C. N. Tadhunter , W. Sparks , D. J. Axon , L. Bergeron , N. J. Jackson , C. Packham , J. H. Hough , A. Robinson , S. Young

We have discovered scattered broad Balmer emission lines in the spectrum of Cygnus A, using the Keck II telescope. Broad H-alpha appears in polarized flux from components on either side of the nucleus, and to a lesser extent in the nucleus.…

天体物理学 · 物理学 2009-10-30 P. M. Ogle , M. H. Cohen , J. S. Miller , H. D. Tran , R. A. E. Fosbury , R. W. Goodrich

We present high-angular (~0.4") resolution mid-infrared (MIR) polarimetric observations in the 8.7 ${\mu}$m and 11.6 ${\mu}$m filters of Cygnus A using CanariCam on the 10.4-m Gran Telescopio CANARIAS. A highly polarized nucleus is observed…

We employ MUSE/VLT data to study the ionised and highly ionised gas phases of the feedback in Circinus, the closest Seyfert 2 galaxy to us. The analysis of the nebular emission allowed us to detect a remarkable high-ionisation gas outflow…

星系天体物理 · 物理学 2021-06-28 M. A. Fonseca-Faria , A. Rodríguez-Ardila , M. Contini , V. Reynaldi

We present subarcsecond resolution mid-infrared images at 10.8 and 18.2 microns of Cygnus A. These images were obtained with the University of Florida mid-IR camera/spectrometer OSCIR at the Keck II 10-m telescope. Our data show extended…

We present preliminary results from high resolution (~ 0.05") adaptive optics observations of Cygnus A. The images show a bi-conic structure strongly suggestive of an obscuring torus around a quasar nucleus. A bright (K'=18.5) point source…

天体物理学 · 物理学 2016-01-27 Gabriela Canalizo , Claire Max , Robert Antonucci , David Whysong , Alan Stockton , Mark Lacy

We detail the spectral analysis of a 170 ks XRISM Resolve observation of the core of Cygnus A. The high spectral resolution of Resolve have enabled us to probe the inner accretion region of Cygnus A by analyzing the 6.4 keV Fe K$\alpha$…

高能天体物理现象 · 物理学 2026-05-19 Anwesh Majumder , T. Heckman , L. Gu , A. Simionescu , B. R. McNamara , A. Ptak , E. Hodges-Kluck , M. Yukita , M. W. Wise , N. Roy

We present the discovery of a 4 kpc molecular gas lane in the Cygnus A host galaxy, using ALMA CO 2-1 observations. The gas lane is oriented roughly perpendicular to the projected radio jet axis. The CO emission generally follows the clumpy…

星系天体物理 · 物理学 2022-10-12 C. L. Carilli , R. A. Perley , D. A. Perley , V. Dhawan , R. Decarli , A. Evans , K. Nyland

We present J, H and K-band images and 0.9-2.5 micron spectra of the nuclear regions of Centaurus A obtained with IRIS on the AAT. While K band has a point source coincident with the nucleus, at H and J we identify diffuse structure…

天体物理学 · 物理学 2009-10-31 J. J. Bryant , R. W. Hunstead

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 spectral analysis on a 170 ks XRISM \textit{Resolve} exposure of the core of Cygnus A. Analyzing the full field of view spectrum in the $1.7-12.0$ keV band, we find evidence for two-temperature cluster gas. The hotter ($kT = 5.53…

高能天体物理现象 · 物理学 2025-12-12 Anwesh Majumder , T. Heckman , J. Meunier , A. Simionescu , B. R. McNamara , L. Gu , A. Ptak , E. Hodges-Kluck , M. Yukita , M. W. Wise , N. Roy

Observations of the oxygen lines [OII]3729 and [OIII]5007 in the medium immediately beyond the Cygnus Loop supernova remnant were carried out with the scanning Fabry-P\'erot spectrophotometer ESOP. Both lines were detected in three…

天体物理学 · 物理学 2009-10-31 J. Bohigas , J. L. Sauvageot , A. Decourchelle

In this paper, we focus on the limb-brightened, prolate spheroidal cavity of the radio galaxy Cygnus A, as revealed by the Chandra X-ray Observatory. We use the shock heated, thermal intracluster medium around the expanding cavity to infer…

天体物理学 · 物理学 2009-11-11 A. S. Wilson , David A. Smith , A. J. Young

We present intermediate resolution near-IR long-slit spectroscopic data for the nearby radio galaxy Cygnus A (3C 405) (obtained with the NIRSPEC spectrograph on the Keck II telescope). The data reveal considerable complexity in the near-IR…

天体物理学 · 物理学 2009-11-10 M. J. Bellamy , C. N. Tadhunter

Our previous studies revealed a good kinematic model for the jet of Cygnus A, but the counter-jet speed is still not well constrained. The central engine and part of the counter-jet of Cyg A are likely to be obscured by free-free absorbing…

天体物理学 · 物理学 2008-12-10 U. Bach , T. P. Krichbaum , E. Middelberg , W. Alef , J. A. Zensus

The prototypical powerful FR \Romannum{2} radio galaxy Cygnus A fits extremely well into the quasar/radio galaxy unified model: high polarization with an angle almost perpendicular to the radio jet and polarized flux showing broad permitted…

星系天体物理 · 物理学 2023-10-31 Atharva Bagul , Patrick Ogle , Robert Antonucci , Philip Maloney , Enrique Lopez-Rodriguez

We present J, H and K-band spectroscopy of Cygnus A, spanning 1.0-2.4 micron in the rest-frame and hence several rovibrational H2, H recombination and [FeII] emission lines. The lines are spatially extended by up to 6kpc from the nucleus,…

天体物理学 · 物理学 2016-08-30 R. J. Wilman , A. C. Edge , R. M. Johnstone , C. S. Crawford , A. C. Fabian

We report Chandra imaging-spectroscopy and RXTE spectroscopy of the nearby, powerful radio galaxy Cygnus A. Various aspects of the results are discussed, including the X-ray properties of the nucleus, the radio hot spots, the cluster of…

天体物理学 · 物理学 2007-05-23 A. S. Wilson , K. A. Arnaud , D. A. Smith , Y. Terashima , A. J. Young
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