Young Globular Formation

The antennae and 2 of its superclusters.

- We can also find virial velocities this high in galaxy mergers.

- Potential formation mechanism for young, metal-rich disk globulars.

- Observational support from the Antennae, in which over 700 young clusters have been found.

- More Observational support found from NGC 1275, gas pileup in LMC?.

Young Globular Formation

The antennae and 2 of its superclusters.

- We can also find virial velocities this high in galaxy mergers. - Potential formation mechanism for young, metal-rich disk globulars. - Observational support from the Antennae, in which over 700 young clusters have been found. - More Observational support found from NGC 1275, gas pileup in LMC?.