The X-ray ribs within the cocoon shock of Cygnus A

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
Přispěvatelé: High Energy Astrophys. & Astropart. Phys (API, FNWI), Sterrenkunde
Rok vydání: 2018
Předmět:
active [Galaxies]
Astrophysics::High Energy Astrophysical Phenomena
galaxies: active
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
galaxies: individual: Cygnus A
0103 physical sciences
Cluster (physics)
Cygnus A
010303 astronomy & astrophysics
Astrophysics::Galaxy Astrophysics
High Energy Astrophysical Phenomena (astro-ph.HE)
Physics
radio continuum: galaxies
Jet (fluid)
Shock (fluid dynamics)
010308 nuclear & particles physics
Astronomy and Astrophysics
Debris
Astrophysics - Astrophysics of Galaxies
Galaxy
galaxies [X-rays]
Core (optical fiber)
Temperature gradient
X-rays: galaxies
galaxies: active
galaxies: individual: Cygnus A
radio continuum: galaxies
X-rays: galaxies
Astrophysics - High Energy Astrophysical Phenomena
Astrophysics - Astrophysics of Galaxies

Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
individual: Cygnus A- radio continuum: galaxies [Galaxies]
Astrophysics - High Energy Astrophysical Phenomena
Zdroj: 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]
ISSN: 1365-2966
0035-8711
Popis: 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 that the X-rays are dominated by thermal emission with an average temperature of around 4 keV, and have discovered an asymmetry in the temperature gradient, with the southwestern part of the gas cooler than the rest by up to 2 keV. Pressure estimates suggest that the gas is a coherent structure of single origin located inside the cocoon, with a mass of roughly $2\times10^{10} M_{\odot}$. We conclude that the gas is debris resulting from disintegration of the cool core of the Cygnus A cluster after the passage of the jet during the early stages of the current epoch of activity. The 4 keV gas now lies on the central inside surface of the hotter cocoon rim. The temperature gradient could result from an offset between the centre of the cluster core and the Cygnus A host galaxy at the switch-on of current radio activity.
15 pages, 12 figures, accepted by MNRAS
Databáze: OpenAIRE