The Globular Cluster System of NGC 5128. II. Ages, Metallicities, Kinematics, and Formation
We present a study of the nearby postmerger giant elliptical galaxy NGC 5128 (Centaurus A), in which we use the properties of its globular cluster (GC) and planetary nebula (PN) systems to constrain its evolution. Using photometric and spectroscopic data
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.