A relatively small cloud of → dust and
→ gas in the → interstellar medium
shaped like a comet with a bright-rimmed head. Cometary globules are situated near
young → massive stars with a strong
→ stellar wind. The wind ionizes gases
on the side facing the → O stars and sweep away the low-density
gas toward the tail. Cometary globules are believed to be
→ molecular cloud
condensations, which are so dense that they are not disrupted when an
→ H II region expands into the molecular cloud surrounding it.
The → Rosette nebula is a good example of an
H II region which shows an abundance of cometary globules.
See also: → comet; → globule.