Zobrazeno 1 - 10
of 136
pro vyhledávání: '"Richard A. Perley"'
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 1, p 16 (2023)
We present the results of a wideband high-resolution polarization study of Hydra A, one of the most luminous FR I radio galaxies known and among the most well studied. The radio emission from this source displays extremely large Faraday rotation meas
Externí odkaz:
https://doaj.org/article/de2008f876084f3e969b2a046c8850b9
Autor:
Valentina Vacca, Federica Govoni, Richard A. Perley, Matteo Murgia, Ettore Carretti, Francesca Loi, Luigina Feretti, Gabriele Giovannini
Publikováno v:
Galaxies, Vol 9, Iss 4, p 112 (2021)
The galaxy cluster Abell 523 hosts a radio halo characterized by the presence of two filaments transversely located with respect to the cluster merger axis. In this paper, we present a spectral index image of these filaments between 1.410 and 1.782 G
Externí odkaz:
https://doaj.org/article/12d26ad7c85941b0927e1e5dd17e3d5e
Autor:
Christopher L. Carilli, Richard A. Perley, Daniel A. Perley, Vivek Dhawan, Roberto Decarli, Aaron S. Evans, Kristina Nyland
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 dust lane
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5938f516811a8c86823cf336ffdbaae1
http://arxiv.org/abs/2209.01278
http://arxiv.org/abs/2209.01278
Autor:
Valentina Vacca, Federica Govoni, Matteo Murgia, Richard A Perley, Luigina Feretti, Gabriele Giovannini, Ettore Carretti, Fabio Gastaldello, Filippo Cova, Paolo Marchegiani, Elia Battistelli, Walter Boschin, Torsten A Enßlin, Marisa Girardi, Francesca Loi, Federico Radiconi
Large-scale magnetic fields reveal themselves through diffuse synchrotron sources observed in galaxy clusters such as radio halos. Total intensity filaments of these sources have been observed in polarization as well, but only in three radio halos ou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64335e1a7c493a1980eb949eecce06e9
http://arxiv.org/abs/2206.03402
http://arxiv.org/abs/2206.03402
Autor:
Julie Hlavacek-Larrondo, Marie-Lou Gendron-Marsolais, A. Richard-Laferrière, Lawrence Rudnick, Emmet Golden-Marx, J. D. McBride, Charles L. H. Hull, Elke Roediger, Richard A. Perley, N. Arakawa, Andrew C. Fabian, R. J. van Weeren, Ralph P. Kraft
Publikováno v:
The Astrophysical Journal, 911(1)
We present new deep, high-resolution, 1.5 GHz observations of the prototypical nearby Perseus galaxy cluster from the Karl G. Jansky Very Large Array. We isolate for the first time the complete tail of radio emission of the bent-jet radio galaxy NGC
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5e443a3d14020d95bc13ee1ec3431cab
http://arxiv.org/abs/2101.05305
http://arxiv.org/abs/2101.05305
Radio interferometric (RI) data are noisy under-sampled spatial Fourier components of the unknown radio sky affected by direction-dependent antenna gains. Failure to model these antenna gains accurately results in a radio sky estimate with limited fi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::35e017c6c2a730d8f20fe415c4cad1f2
Autor:
Amalya C. Johnson, Martijn de Vries, Lerato Sebokolodi, Bradford Snios, Paul Nulsen, Michael W. Wise, Ralph P. Kraft, Richard A. Perley
The powerful FR II radio galaxy Cygnus A exhibits primary and secondary hotspots in each lobe. A 2 Msec Chandra X-ray image of Cygnus A has revealed an approximately circular hole, with a radius of 3.9 kpc, centered on the primary hotspot in the east
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eee90b85905470eafa8e67a680d231a1
http://arxiv.org/abs/2002.02978
http://arxiv.org/abs/2002.02978
Autor:
Alastair C. Edge, Bradford Snios, Michael W. Wise, William G. Mathews, Robert Laing, Martin J. Hardcastle, Paul Nulsen, Ryan T. Duffy, M. N. de Vries, Leith Godfrey, Chris Carilli, D. Rafferty, Mark Birkinshaw, Judith H. Croston, Richard A. Perley, Brian R. McNamara, John McKean, Diana M Worrall
Publikováno v:
Duffy, R T, Worrall, D M, Birkinshaw, M, Nulsen, P E J, Wise, M W, de Vries, M N, Snios, B, Mathews, W G, Perley, R A, Hardcastle, M J, Rafferty, D A, McNamara, B R, Edge, A C, McKean, J P, Carilli, C L, Croston, J H, Godfrey, L E H & Laing, R A 2018, ' The X-ray ribs within the cocoon shock of Cygnus A ', Monthly Notices of the Royal Astronomical Society, vol. 476, no. 4, pp. 4848-4860 . https://doi.org/10.1093/mnras/sty549
Monthly Notices of the Royal Astronomical Society, 476(4), 4848-4860. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2018, Vol.476(4), pp.4848-4860 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 476(4), 4848-4860. Oxford University Press
Monthly notices of the Royal Astronomical Society, 2018, Vol.476(4), pp.4848-4860 [Peer Reviewed Journal]
We use new and archival Chandra observations of Cygnus A, totalling $\sim$1.9 Ms, to investigate the distribution and temperature structure of gas lying within the projected extent of the cocoon shock and exhibiting a rib-like structure. We confirm t
Autor:
Richard A. Perley, Arwa Dabbech, Alexandru Onose, Oleg Smirnov, Abdullah Abdulaziz, Yves Wiaux
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 476:2853-2866
We leverage the Sparsity Averaging Reweighted Analysis (SARA) approach for interferometric imaging, that is based on convex optimisation, for the super-resolution of Cyg A from observations at the frequencies 8.422GHz and 6.678GHz with the Karl G. Ja
Autor:
Hertzog L. Bester, Richard A. Perley, Reimar Leike, Rüdiger Westermann, Torsten A. Enßlin, Oleg Smirnov, Philipp Arras
Publikováno v:
Astronomy & Astrophysics. 646:A84
CLEAN, the commonly employed imaging algorithm in radio interferometry, suffers from a number of shortcomings: In its basic version, it does not have the concept of diffuse flux, and the common practice of convolving the CLEAN components with the CLE