A deep spectroscopic study of the filamentary nebulosity in NGC 4696, the brightest cluster galaxy in the Centaurus cluster

OPTICAL IFU OBSERVATIONS OF THE BRIGHTEST CLUSTER GALAXY NGC 4696: THE CASE FOR A MINOR MERGER AND SHOCK-EXCITED FILAMENTS

(2010) C. L. Farage et al.   ASTROPHYSICAL JOURNAL

Detection of optical coronal emission from 106-K gas in the core of the Centaurus cluster

(2010) R. E. A. Canning et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The diverse nature of optical emission lines in brightest cluster galaxies: IFU observations of the central kiloparsec

(2009) Louise O. V. Edwards et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Collisional heating as the origin of filament emission in galaxy clusters

(2009) G. J. Ferland et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Cool X-ray emitting gas in the core of the Centaurus cluster of galaxies

(2008) J. S. Sanders et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Magnetic support of the optical emission line filaments in NGC 1275

(2008) A. C. Fabian et al.   NATURE