Chemical composition of the young massive cluster NGC 1569-B
Context. The chemical composition of young massive clusters (YMCs) provides stellar population information on their host galaxy. As potential precursors of globular clusters (GCs), their properties can help us understand the origins of GCs and their evolution. Aims: We present a detailed chemical abundance analysis of the YMC NGC 1569-B. The host
Gvozdenko, A. et al.
Fecha de publicación:
10
2022