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Globular clusters lie in the galactic halo, outside of the disc. However, galaxies are more or less a collection of material and objects — why is it, then, that most stars form a plane due to the angular momentum, but some patches of stars do not?

In fact, globular clusters often contain some of the earliest stars formed in a galaxy, right? How come they do not flatten, yet a lot of the older stars do?

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    $\begingroup$ Here's a speculation that other are free to run with if it leads anywhere. Flattening of a gravitational bound system like that requires lots of inelastic interaction between mass elements. That happens faster in a cloud of gas and dust than in a system of discrete and compact objects like stars and planets. Maybe the early formation of starts in those entities simply put them on a longer scale for thermalization of velocities. $\endgroup$ – dmckee Jun 26 '16 at 17:16
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Globular clusters formed whilst the gas of the proto Milky Way was still approximately spherically distributed.

The gas forms a dissipative system that loses energy and collapses (within the first billion years) to a disk whilst conserving angular momentum.

Formed stars and clusters are essentially collisionless so the halo stars continue to have a spherical distribution, whilst more recently formed stars formed from gas already in a disk and so continue to be in a disk.

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