A very deep Chandra view of metals, sloshing and feedback in the Centaurus cluster of galaxies

We examine deep Chandra X-ray observations of the Centaurus cluster of galaxies, Abell 3526. Applying a gradient magnitude filter reveals a wealth of structure, from filamentary soft emission on 100 pc (0.5 arcsec) scales close to the nucleus to features 10 s of kpc in size at larger radii. The clus...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-03, Vol.457 (1), p.82-109
Hauptverfasser:	Sanders, J. S., Fabian, A. C., Taylor, G. B., Russell, H. R., Blundell, K. M., Canning, R. E. A., Hlavacek-Larrondo, J., Walker, S. A., Grimes, C. K.
Format:	Artikel
Sprache:	eng
Schlagworte:	Clusters Correlation Galactic clusters Holes Kelvin-Helmholtz instability Metallicity Nuclei Sound waves Star & galaxy formation Surface brightness Turbulence X-ray astronomy
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