A single population of red globular clusters around the massive compact galaxy NGC 1277
Massive galaxies are thought to form in two phases: an initial collapse of gas and giant burst of central star formation, followed by the later accretion of material that builds up their stellar and dark-matter haloes. The systems of globular clusters within such galaxies are believed to form in a similar manner. The initial central burst forms
Beasley, M. A. et al.
Fecha de publicación:
3
2018