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McDermid (2, Rob Sharp (8) ((1) Centre for Astrophysics & Supercomputing, Sarah Brough (2), Stanford University. (7) Department of Physics, Stanford University. (8) Research School of Astronomy & Astrophysics, Swinburne University of Technology. (2) Australian Astronomical Observatory. (3) George P., Texas A&M University. (4) Department of Physics & Astronomy, University of Copenhagen. (6) Kavli Institute for Particle Astrophysics, Warrick J. Couch (1","submitted_at":"2015-03-04T21:00:18Z","abstract_excerpt":"We analyse the spatially-resolved stellar populations of 9 local ($z<0.1$) Brightest Cluster Galaxies (BCGs) observed with VIMOS in IFU mode. Our sample is composed of 7 slow-rotating and 2 fast-rotating BCGs. We do not find a connection between stellar kinematics and stellar populations in this small sample. 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