Some are found in globular clusters, but
most move in a huge cloud around the
disk called the
galactic halo, which has a luminous inner component defined by globular star clusters and other easily observable stars (with coronae of hot gas possibly expelled by supernovae and of high - velocity neutron stars) and an outer dark - matter component inferred from its gravitational impact on the Milky Way's spiral
disk.
Because gravity depends upon mass, you might think that
most of a galaxy's mass would lie in the
galactic disk or near the center of the
disk.