The SAMI Galaxy Survey : mass as the driver of the kinematic morphology - density relation in clusters

We examine the kinematic morphology of early-type galaxies (ETGs) in eight galaxy clusters in the Sydney-AAO Multi-object Integral-field spectrograph Galaxy Survey. The clusters cover a mass range of 14.2 < log(M_(200)/M_☉) < 15.2 and we measure spatially resolved stellar kinematics for 315 member galaxies with stellar masses 10.0

Keywords:

• Substructure
• Stellar kinematics
• Stellar mass
• Astrophysics
• Cluster (physics)
• Galaxy
• Mass segregation
• Physics
• Galaxy cluster
• Population

• Correction
• Source
• Cite
• Save
• Machine Reading By IdeaReader