HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster

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HST imaging of the dusty filaments and nucleus swirl in NGC4696 at the centre of the Centaurus Cluster

Narrow-band HST imaging has resolved the detailed internal structure of the 10 kpc diameter H α+[N II] emission line nebulosity in NGC4696, the central galaxy in the nearby Centaurus cluster, showing that the dusty, molecular, filaments have a width of about 60 pc. Optical morphology and velocity me...

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Bibliographic Details
Main Authors:	Fabian, A.C., Walker, S.A., Russell, H.R., Pinto, C., Canning, R.E.A., Salome, P., Sanders, J.S., Taylor, G.B., Zweibel, E.G., Conselice, Christopher J., Combes, F., Crawford, C.S., Ferland, G.J., Gallager, J.S., Hatch, Nina A., Johnstone, R.M., Reynolds, C.S.
Format:	Article
Published:	Oxford University Press 2016
Subjects:	black hole physics galaxies:clusters:individual:GGC4696 galaxies:clusters:intracluster medium x-rays:galaxies
Online Access:	https://eprints.nottingham.ac.uk/37221/

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